|
astro-ph/9409087 🔍 (source)
|
cluster mass |
|
66000.0 ± 5000.0 |
|
|
astro-ph/9507008 🔍 (source)
|
cluster mass-to-light ratio |
|
440.0 ± 80.0 h M_\odot L_\odot-1 |
|
|
astro-ph/9603076 🔍 (source)
|
cluster distance |
m - M |
31.79 ± 0.09 |
|
|
astro-ph/9603076 🔍 (source)
|
cluster velocity |
|
1178.0 ± 32.0 km s-1 |
|
|
astro-ph/9604020 🔍 (source)
|
amplitude of clustering |
\sigma _ { 8 } |
0.7 ± 0.05 |
|
|
astro-ph/9604032 🔍 (source)
|
locus of cluster ellipticals shifts monotonically |
|
-0.55 ± 0.12 |
|
|
astro-ph/9604150 🔍 (source)
|
cluster temperature |
|
9.0 keV |
|
|
astro-ph/9604159 🔍 (source)
|
globular cluster specific frequency |
S _ { N } |
9.0 |
|
|
astro-ph/9604179 🔍 (source)
|
distance to the cluster |
{ ( m - M ) } _ { \circ } |
13.05 |
|
|
astro-ph/9605013 🔍 (source)
|
cluster binary fraction |
x _ { b } |
0.01 +0.1-0.01 |
|
|
astro-ph/9605040 🔍 (source)
|
globular cluster density profile |
|
-1.3 ± 0.4 |
|
|
astro-ph/9605056 🔍 (source)
|
clustering length |
r _ { 0 } |
1.86 ± 0.43 Mpc |
|
|
astro-ph/9605099 🔍 (source)
|
absolute age of the globular clusters |
|
14.6 ± 1.7 Gyr |
|
|
astro-ph/9606116 🔍 (source)
|
galaxy clustering |
A _ { G } |
14.5 +3.8-3.0 |
|
|
astro-ph/9607063 🔍 (source)
|
total mass of the cluster |
|
450000000000000.0 M_\odot |
|
|
astro-ph/9607063 🔍 (source)
|
total mass of the cluster |
|
2349999999999999.5 +950000000000000.1-949999999999999.8 M_\odot |
|
|
astro-ph/9608116 🔍 (source)
|
galaxy cluster abundance |
|
0.13 |
|
|
astro-ph/9608116 🔍 (source)
|
galaxy cluster abundance |
\Delta _ { \tau _ { 0 } } |
0.058 |
|
|
astro-ph/9608167 🔍 (source)
|
age of the cluster |
E ( B - V ) |
0.275 +0.044999999999999984-0.04500000000000001 |
|
|
astro-ph/9609176 🔍 (source)
|
mean cluster metallicity |
[ Fe / H ] |
-0.7 ± 0.3 |
|
|
astro-ph/9609176 🔍 (source)
|
cluster velocity dispersion |
|
260.0 km s-1 |
|
|
astro-ph/9612190 🔍 (source)
|
clustering signal |
\theta |
0.01 |
|
|
astro-ph/9612190 🔍 (source)
|
clustering signal |
w ( \theta ) |
0.01 |
|
|
astro-ph/9701179 🔍 (source)
|
cluster luminosity |
L _ { X } ^ { \star } |
1.8 |
Upper |
|
astro-ph/9706128 🔍 (source)
|
mean age of the oldest globular clusters |
|
11.5 ± 1.3 Gyr |
|
|
astro-ph/9708120 🔍 (source)
|
number of identifiable microlensing events per nearby cluster |
|
0.02 |
|
|
astro-ph/9709040 🔍 (source)
|
mean cluster distance |
{ ( m - M ) } ^ { 0 } |
31.0 |
|
|
astro-ph/9709040 🔍 (source)
|
mean distance of subcluster A |
|
0.0 |
|
|
astro-ph/9709040 🔍 (source)
|
cluster velocity |
|
1142.0 ± 61.0 km s-1 |
|
|
astro-ph/9709270 🔍 (source)
|
mass of the supercluster |
|
7600000000000000.0 ± 2000000000000000.0 M_\odot h-1 |
|
|
astro-ph/9709270 🔍 (source)
|
supercluster luminosity |
|
14000000000000.0 ± 2000000000000.0 L_\odot h-2 |
|
|
astro-ph/9711246 🔍 (source)
|
cluster-galaxy correlation lengths |
|
7.2 ± 0.5 Mpc h-1 |
|
|
astro-ph/9801120 🔍 (source)
|
cluster velocity dispersion |
|
1213.0 +352.0-191.0 km s-1 |
|
|
astro-ph/9801137 🔍 (source)
|
cluster velocity |
|
32.0 ± 7.0 % |
|
|
astro-ph/9803099 🔍 (source)
|
surface density of clusters |
|
0.57 ± 0.07 s-1 |
|
|
astro-ph/9803167 🔍 (source)
|
age outer disk clusters |
[ Fe/H ] > |
-0.7 |
|
|
astro-ph/9806177 🔍 (source)
|
mean intercluster separation |
d _ { cl } |
30.0 Mpc h-1 |
|
|
astro-ph/9807057 🔍 (source)
|
mean cluster radial velocity |
|
-54.9 ± 0.12 km s-1 |
|
|
astro-ph/9807298 🔍 (source)
|
clustered-mass density parameter |
\Omega _ { 0 } |
0.55 +0.44999999999999996-0.45000000000000007 |
|
|
astro-ph/9808038 🔍 (source)
|
cluster velocity dispersion |
|
530.0 km s-1 |
|
|
astro-ph/9808180 🔍 (source)
|
intracluster gas/cluster |
|
152.0 |
|
|
astro-ph/9808353 🔍 (source)
|
mean cluster reddening |
E ( B - V ) |
0.45 ± 0.03 mag |
|
|
astro-ph/9812218 🔍 (source)
|
integrated rest-frame luminosity of the cluster |
L _ { V } |
320000000000.0 L_\odot h-2 |
Lower |
|
astro-ph/9812283 🔍 (source)
|
cluster distance |
|
2.35 kpc |
|
|
astro-ph/9812477 🔍 (source)
|
average intracluster temperature |
|
9.0 keV |
|
|
astro-ph/9901062 🔍 (source)
|
cluster baryon fraction |
|
5.0 |
|
|
astro-ph/9902035 🔍 (source)
|
cluster |
M _ { tot } ) |
919999999999999.9 ± 270000000000000.03 M_\odot |
|
|
astro-ph/9903194 🔍 (source)
|
X-ray-emitting intracluster medium |
|
0.25 ± 0.14 s |
|
|
astro-ph/9903324 🔍 (source)
|
total numbers of globular clusters |
N _ { GC } ( 4565 ) |
204.0 ± 38.0 +87.0-53.0 |
|
|
astro-ph/9903457 🔍 (source)
|
cluster mass |
M |
6000000.0 |
|
|
astro-ph/9904382 🔍 (source)
|
cluster average temperatures |
|
4.8 ± 0.2 keV |
|
|
astro-ph/9904382 🔍 (source)
|
cluster average temperatures |
|
4.7 ± 0.2 keV |
|
|
astro-ph/9905139 🔍 (source)
|
resulting total mass of the cluster |
M ( r < 1 Mpc ) |
1000000000000000.0 ± 300000000000000.0 M_\odot |
|
|
astro-ph/9905281 🔍 (source)
|
cluster mass |
\Omega _ { h } |
0.26 |
|
|
astro-ph/9906295 🔍 (source)
|
cluster |
|
210000000000000.0 +150000000000000.0-80000000000000.0 M_\odot h-1 |
|
|
astro-ph/9912108 🔍 (source)
|
AGN clustering amplitude |
A |
98.0 ± 54.0 |
|
|
astro-ph/9912108 🔍 (source)
|
quasar clustering amplitude |
|
3.7 ± 2.0 |
|
|
astro-ph/9912162 🔍 (source)
|
supercluster |
|
600.0 Myr |
|
|
astro-ph/9912153 🔍 (source)
|
clustering strength |
|
1.0 |
|
|
astro-ph/9912481 🔍 (source)
|
young cluster age |
|
50.0 Myr s |
|
|
astro-ph/0002205 🔍 (source)
|
globular cluster metallicity range |
[ Fe / H ] |
-2.2 |
Lower |
|
astro-ph/0002530 🔍 (source)
|
cluster radius |
|
0.6 pc |
|
|
astro-ph/0003440 🔍 (source)
|
cluster proper motion |
|
-3.2 ± 0.6 m as yr-1 |
|
|
astro-ph/0004012 🔍 (source)
|
cluster radial velocity |
|
1987.0 |
|
|
astro-ph/0006299 🔍 (source)
|
globular cluster metallicity range |
[ Fe / H ] |
-2.2 |
Lower |
|
astro-ph/0009382 🔍 (source)
|
average clustercentric distance |
|
580.0 kpc |
|
|
astro-ph/0009401 🔍 (source)
|
mean reddening of the cluster |
E ( B - V ) |
0.32 ± 0.03 |
|
|
astro-ph/0011125 🔍 (source)
|
cluster |
{ [ Fe / H ] } _ { M 35 } |
-0.21 ± 0.1 |
|
|
astro-ph/0012175 🔍 (source)
|
cluster X-ray luminosity function |
L _ { X } |
5.0000000000000004e+44 h |
Lower |
|
astro-ph/0101486 🔍 (source)
|
cluster distance |
|
320.0 pc |
|
|
astro-ph/0102113 🔍 (source)
|
metal–rich clusters peak |
[ Fe / H ] |
-0.6 dex |
|
|
astro-ph/0102260 🔍 (source)
|
cluster |
m - M |
34.94 ± 0.13 mag |
|
|
astro-ph/0102260 🔍 (source)
|
cluster |
H _ { 0 } |
73.0 ± 4.0 km s-1 Mpc-1 |
|
|
astro-ph/0103041 🔍 (source)
|
cluster temperature |
kT |
2.3 +1.8-0.8 keV |
|
|
astro-ph/0104133 🔍 (source)
|
total cluster mass |
|
65.0 pc |
|
|
astro-ph/0104133 🔍 (source)
|
total cluster mass |
|
1700000.0 ± 900000.0 |
|
|
astro-ph/0104164 🔍 (source)
|
cluster extent |
R |
9.0 |
|
|
astro-ph/0104397 🔍 (source)
|
cluster velocity dispersion |
\sigma |
1000.0 km s-1 |
|
|
astro-ph/0106261 🔍 (source)
|
cluster distance |
|
18.0 ± 1.2 Mpc |
|
|
astro-ph/0107341 🔍 (source)
|
reddening of the cluster |
E ( \bv ) |
0.51 ± 0.02 mag |
|
|
astro-ph/0107373 🔍 (source)
|
mean H I mass-to-light ratio of the cluster galaxies |
|
0.68 ± 0.15 |
|
|
astro-ph/0107491 🔍 (source)
|
total globular cluster population |
|
1590.0 ± 854.0 |
|
|
astro-ph/0108277 🔍 (source)
|
cluster temperature |
T _ { e } |
2.09 +0.83-0.54 keV |
|
|
astro-ph/0109099 🔍 (source)
|
mean cluster age |
|
5.0 Myr |
Upper |
|
astro-ph/0109263 🔍 (source)
|
mean cluster temperature |
kT |
6.9 ± 0.5 |
|
|
astro-ph/0109488 🔍 (source)
|
total cluster mass |
|
2.0 |
Lower |
|
astro-ph/0109488 🔍 (source)
|
total cluster mass |
|
279999999999999.97 M_\odot |
|
|
astro-ph/0110066 🔍 (source)
|
supercluster |
|
600.0 Myr |
|
|
astro-ph/0111019 🔍 (source)
|
clustering lengths |
|
4.2 ± 0.4 Mpc h-1 |
|
|
astro-ph/0111019 🔍 (source)
|
clustering lengths |
r _ { 0 } |
7.8 ± 0.7 Mpc h-1 |
|
|
astro-ph/0111285 🔍 (source)
|
cluster masses |
\Omega _ { Cluster } |
0.012 +0.003-0.004 |
|
|
astro-ph/0111285 🔍 (source)
|
cluster masses |
|
64000000000000.0 +7000000000000.0-6000000000000.0 h |
Upper |
|
astro-ph/0201069 🔍 (source)
|
supercluster |
z |
0.07 |
Upper |
|
astro-ph/0201181 🔍 (source)
|
clustering amplitude |
r _ { o } |
11.5 ± 3.0 ± 3.0 Mpc h-1 |
|
|
astro-ph/0201486 🔍 (source)
|
cluster mass |
|
-3000000.0 M_\odot |
|
|
astro-ph/0202319 🔍 (source)
|
total cluster mass |
|
2.0 |
Lower |
|
astro-ph/0202319 🔍 (source)
|
total cluster mass |
|
279999999999999.97 M_\odot |
|
|
astro-ph/0203157 🔍 (source)
|
cluster age |
|
11.0 ± 1.4 Gyr |
|
|
astro-ph/0203166 🔍 (source)
|
intercluster separation |
d _ { cl } |
50.0 Mpc h-1 |
|
|
astro-ph/0204306 🔍 (source)
|
cluster mean temperature |
k T |
5.3 ± 0.5 keV |
|
|
astro-ph/0205490 🔍 (source)
|
cluster normalization relation |
|
0.33 ± 0.03 |
|
|
astro-ph/0205490 🔍 (source)
|
cluster normalization relation |
\sigma _ { 8 } \Omega _ { m } ^ { 0.6 } |
0.1 |
Lower |
|
astro-ph/0206442 🔍 (source)
|
cluster velocity dispersion |
|
1016.0 +126.0-93.0 km s-1 |
|
|
astro-ph/0208428 🔍 (source)
|
mean metallicity of the globular cluster |
[ Fe / H ] |
-1.6 ± 0.1 dex |
|
|
astro-ph/0211002 🔍 (source)
|
color of these clusters |
{ ( V - I ) } _ { o } |
1.04 |
|
|
astro-ph/0211030 🔍 (source)
|
cluster |
[ Fe / H ] |
-1.58 ± 0.28 |
|
|
astro-ph/0211030 🔍 (source)
|
cluster |
|
3.5 ± 0.5 Gyr |
|
|
astro-ph/0211230 🔍 (source)
|
mean cluster gas temperature |
kT |
4.46 +0.14-0.15 |
|
|
astro-ph/0211420 🔍 (source)
|
real cluster formation rates in the pre-burst phase |
|
9.4 |
Lower |
|
astro-ph/0211420 🔍 (source)
|
real cluster formation rates in the pre-burst phase |
\log ( t / { yr } |
8.4 |
Lower |
|
astro-ph/0211420 🔍 (source)
|
real cluster formation rates in the pre-burst phase |
\log ( t / yr ) |
8.4 |
Lower |
|
astro-ph/0211566 🔍 (source)
|
cluster galaxies |
\langle z _ { \star } ^ { cl } \rangle |
2.0 +0.3-0.2 |
|
|
astro-ph/0212375 🔍 (source)
|
redshift-space clustering length |
s _ { 0 } |
6.82 ± 0.28 Mpc h-1 |
|
|
astro-ph/0301469 🔍 (source)
|
total cluster mass |
M |
8000000.0 ± 1000000.0 M_\odot |
|
|
astro-ph/0301529 🔍 (source)
|
cluster distance |
d |
2750.0 ± 250.0 pc |
|
|
astro-ph/0303083 🔍 (source)
|
cluster age |
|
54.0 Myr |
|
|
astro-ph/0303221 🔍 (source)
|
cluster mean |
Fe/H ] |
0.13 ± 0.01 |
|
|
astro-ph/0303429 🔍 (source)
|
cluster of size |
r |
3.9 pc |
|
|
astro-ph/0303587 🔍 (source)
|
cluster center |
\tau _ { 0 } |
0.00535 ± 0.00067 |
|
|
astro-ph/0304483 🔍 (source)
|
rich cluster mass profile |
D _ { NBDM } |
6e+28 m2 s-1 |
|
|
astro-ph/0305184 🔍 (source)
|
cluster disruption time-scales |
\log ( t _ { 4 } ^ { dis } / yr ) |
8.05 |
|
|
astro-ph/0305184 🔍 (source)
|
cluster disruption time-scales |
\log ( t _ { 4 } ^ { dis } / yr ) |
7.75 |
Lower |
|
astro-ph/0305318 🔍 (source)
|
globular-cluster age |
|
12.25 ± 1.25 Gyr |
|
|
astro-ph/0305603 🔍 (source)
|
clustering length |
r _ { 0 } |
5.77 ± 0.1 Mpc h-1 |
|
|
astro-ph/0305606 🔍 (source)
|
comptonization parameter associated to supercluster scales |
y _ { SC } |
2.1800000000000003e-08 |
Upper |
|
astro-ph/0305603 🔍 (source)
|
clustering length |
|
4.51 ± 0.19 Mpc h-1 |
|
|
astro-ph/0307223 🔍 (source)
|
cluster temperature |
|
5.5 ± 0.5 keV |
|
|
astro-ph/0308024 🔍 (source)
|
intracluster Fe abundance |
|
0.36 +0.040000000000000036-0.03999999999999998 |
|
|
astro-ph/0308287 🔍 (source)
|
clusters |
z |
0.5 |
Lower |
|
astro-ph/0309196 🔍 (source)
|
total cluster mass |
M _ { total } |
1800.0 ± 200.0 M_\odot |
Upper |
|
astro-ph/0309196 🔍 (source)
|
cluster age |
|
2.0 ± 1.0 Myr |
|
|
astro-ph/0310174 🔍 (source)
|
mass clustering amplitude |
{ \sigma _ { 8 } ( \Omega _ { m } / 0.27 ) } ^ { 0.6 } |
0.71 ± 0.11 |
|
|
astro-ph/0310317 🔍 (source)
|
cluster galaxies |
|
100000000000.0 L_\odot |
|
|
astro-ph/0310533 🔍 (source)
|
QSO clustering |
s _ { 0 } |
5.76 +0.17-0.27 Mpc h-1 |
|
|
astro-ph/0311232 🔍 (source)
|
cluster luminosity |
M _ { V } |
-16.2 |
|
|
astro-ph/0311232 🔍 (source)
|
cluster size |
R _ { eff } |
17.5 ± 1.8 pc |
|
|
astro-ph/0311402 🔍 (source)
|
cluster emission-weighted mean temperature |
|
11.8 ± 0.6 keV |
|
|
astro-ph/0312083 🔍 (source)
|
total cluster mass |
M |
1300.0 ± 90.0 ± 170.0 M_\odot |
|
|
astro-ph/0312160 🔍 (source)
|
redshift-space clustering length |
s _ { 0 } |
10.7 +0.8-0.7 Mpc |
|
|
astro-ph/0312215 🔍 (source)
|
mean galaxy-HLIRG clustering amplitude |
\langle B _ { gh } \rangle |
190.0 ± 45.0 Mpc |
|
|
astro-ph/0403423 🔍 (source)
|
clustering |
x _ { 0 } |
5.0 ± 0.3 Mpc h-1 |
|
|
astro-ph/0405092 🔍 (source)
|
cluster frame to amount |
|
1700.0 ± 150.0 km s-1 |
|
|
astro-ph/0405234 🔍 (source)
|
mass-to-light ratios of rich clusters |
|
0.7 |
|
|
astro-ph/0405234 🔍 (source)
|
mass-to-light ratios of rich clusters |
\sigma _ { 8 } |
0.9 |
|
|
astro-ph/0406036 🔍 (source)
|
linear mass-clustering amplitude |
\sigma _ { 8 } |
0.8 |
|
|
astro-ph/0407567 🔍 (source)
|
cluster mass |
|
5600.0 M_\odot |
|
|
astro-ph/0408028 🔍 (source)
|
cluster velocity dispersion |
\sigma _ { V } |
775.0 +182.0-113.0 km s-1 |
|
|
astro-ph/0408028 🔍 (source)
|
cluster X-ray bolometric luminosity |
L _ { BOL , X } |
1.35e+45 +7.999999999999999e+43-2.1e+44 h |
|
|
astro-ph/0408043 🔍 (source)
|
cluster formation rate |
|
60.0 ± 10.0 Myr |
Lower |
|
astro-ph/0409269 🔍 (source)
|
cluster ’ s binary fraction |
|
30.0 ± 4.0 % |
|
|
astro-ph/0409362 🔍 (source)
|
cluster distance |
|
118.0 pc |
|
|
astro-ph/0409447 🔍 (source)
|
cluster age |
|
150.0 Myr |
|
|
astro-ph/0409627 🔍 (source)
|
overall temperature of the cluster |
kT |
10.0 ± 0.3 keV |
|
|
astro-ph/0410642 🔍 (source)
|
enclosed cluster mass |
M ( \langle 360 \rangle h ^ { -1 } kpc ) |
1200000000000000.0 ± 300000000000000.0 M_\odot |
|
|
astro-ph/0411432 🔍 (source)
|
spatial clustering of EROs decreases |
r _ { 0 } |
9.7 ± 1.1 Mpc h-1 |
|
|
astro-ph/0411432 🔍 (source)
|
spatial clustering |
r _ { 0 } |
9.7 ± 1.1 Mpc h-1 |
|
|
astro-ph/0411572 🔍 (source)
|
clustering length |
r _ { o } |
-17.0 Mpc h-1 |
|
|
astro-ph/0501560 🔍 (source)
|
cluster age |
|
3.75 ± 0.75 Myr |
|
|
astro-ph/0502292 🔍 (source)
|
cluster radius |
|
5.0 ± 1.0 |
|
|
astro-ph/0502292 🔍 (source)
|
cluster total mass |
|
2570.0 ± 210.0 M_\odot |
|
|
astro-ph/0503250 🔍 (source)
|
line-of-sight cluster magnetic |
B _ { \| } |
2.1 |
|
|
astro-ph/0503509 🔍 (source)
|
clustering parameter |
b |
0.867 ± 0.026 |
|
|
astro-ph/0504335 🔍 (source)
|
cluster frequency |
S _ { N } |
1.3 ± 0.6 |
|
|
astro-ph/0504439 🔍 (source)
|
cluster age |
|
150.0 ± 50.0 Myr |
|
|
astro-ph/0505104 🔍 (source)
|
number of young/intermediate age clusters |
|
2.0 Gyr |
|
|
astro-ph/0505408 🔍 (source)
|
specific frequency of globular clusters |
S _ { N } |
0.4 |
|
|
astro-ph/0506066 🔍 (source)
|
cluster formation rate |
|
3.0 +4.6-1.2 |
|
|
astro-ph/0506394 🔍 (source)
|
cluster temperature |
|
5.2 +1.2-0.9 keV |
|
|
astro-ph/0506493 🔍 (source)
|
cluster age |
|
0.5 Gyr s |
|
|
astro-ph/0508575 🔍 (source)
|
scale height of open clusters |
|
56.0 ± 3.0 pc |
|
|
astro-ph/0510144 🔍 (source)
|
cluster age |
|
0.06 ± 0.02 |
|
|
astro-ph/0510168 🔍 (source)
|
unweighted mean cluster distance |
|
18.3 ± 0.05 |
|
|
astro-ph/0510484 🔍 (source)
|
cluster metallicity |
[ Fe / H ] |
0.067 |
|
|
astro-ph/0510721 🔍 (source)
|
mean cluster O abundance |
[ O / H ] |
0.12 ± 0.02 |
|
|
astro-ph/0511305 🔍 (source)
|
characteristic cluster disruption time-scale |
\log ( t _ { 4 } ^ { dis } / yr ) |
9.9 ± 0.1 |
|
|
astro-ph/0511522 🔍 (source)
|
cluster radius |
|
3.4 pc |
|
|
astro-ph/0511553 🔍 (source)
|
cluster age |
|
89130000.0 yr |
|
|
astro-ph/0511717 🔍 (source)
|
slope of the cluster IMF |
x |
1.8 ± 0.2 |
|
|
astro-ph/0512233 🔍 (source)
|
clustering scale-length |
|
3.69 ± 0.14 |
|
|
astro-ph/0512233 🔍 (source)
|
clustering scale-length |
r _ { 0 } |
4.43 ± 0.14 |
|
|
astro-ph/0512297 🔍 (source)
|
cluster mass |
M _ { max } |
1900000.0 +600000.0000000001-599999.9999999999 |
|
|
astro-ph/0601294 🔍 (source)
|
mean cluster reddening |
E ( V - I ) |
0.4 ± 0.03 |
|
|
astro-ph/0601700 🔍 (source)
|
temperature of the lensing cluster |
|
4.700000000000001e+44 erg s-1 |
|
|
astro-ph/0602019 🔍 (source)
|
cluster-centric |
|
99.7 % |
Upper |
|
astro-ph/0603192 🔍 (source)
|
cluster mass |
|
1900000000000000.0 ± 500000000000000.0 M_\odot |
|
|
astro-ph/0603314 🔍 (source)
|
cluster age |
|
625.0 ± 50.0 Myr s |
|
|
astro-ph/0603349 🔍 (source)
|
areal density of blue globular clusters falls to 30 per cent |
|
45.0 ± 5.0 |
|
|
astro-ph/0603768 🔍 (source)
|
cluster age |
|
20.0 |
|
|
astro-ph/0603768 🔍 (source)
|
cluster age |
|
50.0 Myr |
Upper |
|
astro-ph/0604140 🔍 (source)
|
cluster masses |
|
6.25 ± 0.21 |
|
|
astro-ph/0604140 🔍 (source)
|
cluster masses |
\overline { \log M } |
7.63 ± 0.24 |
|
|
astro-ph/0606138 🔍 (source)
|
intrinsic cluster depth |
\sigma _ { int } |
0.74 |
|
|
astro-ph/0606734 🔍 (source)
|
mean distance to the cluster |
|
10.49 ± 0.15 kpc |
|
|
astro-ph/0607052 🔍 (source)
|
cluster velocities |
|
1.6 km s-1 |
|
|
astro-ph/0607559 🔍 (source)
|
cluster redshift |
|
-13.0 |
Lower |
|
astro-ph/0607597 🔍 (source)
|
kinematic distance to the cluster |
D |
4.0 ± 0.35 kpc |
|
|
astro-ph/0609162 🔍 (source)
|
Galactic globular cluster ages |
|
15.0 Gyr |
|
|
astro-ph/0609749 🔍 (source)
|
superclusters |
M _ { bj } |
-21.02 |
|
|
astro-ph/0610793 🔍 (source)
|
cluster distance |
|
6.2 ± 1.2 kpc |
|
|
astro-ph/0610921 🔍 (source)
|
galaxy ’ s velocity relative to the intra-cluster medium |
|
-550.0 km s-1 |
Upper |
|
astro-ph/0611164 🔍 (source)
|
young cluster IMF |
|
0.3 ± 0.1 |
|
|
astro-ph/0611409 🔍 (source)
|
comoving clustering length |
r _ { 0 } |
14.0 +2.1-2.4 Mpc |
|
|
astro-ph/0612190 🔍 (source)
|
clustering |
b _ { Q } ^ { \bar { z } |
2.41 ± 0.08 |
|
|
astro-ph/0612360 🔍 (source)
|
total cluster flux |
|
3.0000000000000002e-15 erg cm-2 s-1 |
|
|
astro-ph/0612463 🔍 (source)
|
specific frequency of globular clusters |
S _ { N } |
1.65 ± 0.25 |
|
|
astro-ph/0701649 🔍 (source)
|
cluster metallicity |
|
-0.37 dex |
|
|
astro-ph/0703075 🔍 (source)
|
distance of young clusters |
|
2.0 kpc |
Lower |
|
astro-ph/0703075 🔍 (source)
|
distance of young clusters |
|
-47.0 ± 16.0 pc |
|
|
astro-ph/0703580 🔍 (source)
|
\it intracluster |
|
5.008 ± 0.005 |
|
|
0704.3739 🔍 (source)
|
amplitude of LRG clustering |
s _ { 0 } |
9.9 ± 0.7 Mpc h-1 |
|
|
0706.4371 🔍 (source)
|
clustering length |
r _ { 0 } |
2.76 +0.17-0.15 Mpc h-1 |
|
|
0707.4655 🔍 (source)
|
ellipticity of the cluster |
\epsilon |
0.14 ± 0.03 |
|
|
0708.3671 🔍 (source)
|
integrated cluster temperature |
|
5.1 +0.9-0.5 keV |
|
|
0708.3671 🔍 (source)
|
cluster cooling time |
|
3300000000.0 yr s |
|
|
0709.3063 🔍 (source)
|
total cluster mass |
|
3640.0 ± 170.0 M_\odot |
|
|
0710.0878 🔍 (source)
|
clusters |
f _ { cl } |
0.001 |
Lower |
|
0710.0953 🔍 (source)
|
cluster age |
|
1400000000.0 yr s |
|
|
0711.0843 🔍 (source)
|
angular clustering strength |
A |
0.014745 +0.014255-0.014254999999999999 |
|
|
0711.1779 🔍 (source)
|
total dynamical cluster mass |
|
125000.0 M_\odot |
|
|
0712.0226 🔍 (source)
|
cluster age |
|
27.7 +4.2-3.5 ± 1.1 ± 2.0 Myr |
|
|
0712.1819 🔍 (source)
|
spatial–clustering scale length |
r _ { 0 } |
22.4 ± 3.6 Mpc h-1 |
|
|
0801.0968 🔍 (source)
|
hot diffuse intracluster plasma |
|
20.0 |
Upper |
|
0802.0815 🔍 (source)
|
cluster distance modulus |
|
14.7 ± 0.35 mag |
|
|
0803.0598 🔍 (source)
|
cluster redshift path |
\Delta z _ { cluster } |
6.3 |
|
|
0804.0502 🔍 (source)
|
average redshift of the cluster |
|
0.268 |
|
|
0804.3448 🔍 (source)
|
number density of the cluster |
|
2.2e-07 Mpc-3 |
|
|
0804.3590 🔍 (source)
|
cluster mean |
Fe / H |
0.1 |
|
|
0804.4143 🔍 (source)
|
cluster age |
|
4.0 ± 1.0 Myr |
|
|
0805.1189 🔍 (source)
|
cluster age |
|
625.0 Myr |
|
|
0805.3817 🔍 (source)
|
cluster mass |
M _ { 500 } |
559999999999999.94 M_\odot |
|
|
0806.1575 🔍 (source)
|
total cluster mass |
M _ { 500 } |
1190000000000000.0 ± 350000000000000.0 M_\odot |
|
|
0807.0092 🔍 (source)
|
cluster distance modulus |
|
9.63 |
|
|
0807.1085 🔍 (source)
|
cluster distance modulus |
|
9.63 ± 0.08 |
|
|
0807.3744 🔍 (source)
|
farthest cluster |
|
38.0 |
|
|
0807.3744 🔍 (source)
|
farthest cluster |
Lindsay |
67.0 kpc |
|
|
0807.4208 🔍 (source)
|
mass-weighted temperature of the cluster gas |
T _ { mg } |
10.8 ± 0.9 keV |
|
|
0807.4573 🔍 (source)
|
cluster age |
|
7.0 ± 1.0 Myr |
|
|
0807.4573 🔍 (source)
|
kinematic cluster distance |
|
4.7 ± 0.4 kpc |
|
|
0808.0018 🔍 (source)
|
mean cluster velocities |
|
2.7 km s-1 |
|
|
0808.0354 🔍 (source)
|
distance to the cluster |
|
2.8 ± 0.1 kpc |
|
|
0808.0354 🔍 (source)
|
distance to the cluster |
d |
2.7 ± 0.1 kpc |
|
|
0809.2853 🔍 (source)
|
lifetime of the intracluster dust inferred |
|
5.0 Myr |
Upper |
|
0809.3737 🔍 (source)
|
cluster age |
|
5.0 ± 0.5 Gyr |
|
|
0809.4188 🔍 (source)
|
average distance to the cluster |
|
156.0 ± 24.0 pc |
|
|
0809.4320 🔍 (source)
|
cluster velocity dispersion |
|
3.6 |
Lower |
|
0810.0709 🔍 (source)
|
total mass of the cluster |
M ( r < r _ { 200 } ) |
1400000000000000.0 ± 200000000000000.0 M_\odot |
|
|
0810.2407 🔍 (source)
|
apparent cluster distance-modulus |
{ ( m - M ) } _ { V } |
13.46 ± 0.1 |
|
|
0810.3584 🔍 (source)
|
average cluster age |
|
1.0 Myr |
Upper |
|
0811.3031 🔍 (source)
|
cluster redshift |
z |
0.0553 ± 0.0002 |
|
|
0812.1699 🔍 (source)
|
cluster redshift |
z |
1.84 |
Lower |
|
0812.2021 🔍 (source)
|
projected clustercentric radii |
R |
3.0 Mpc |
Lower |
|
0901.0773 🔍 (source)
|
cluster mean age |
|
1.35 +0.11-0.04 Gyr |
|
|
0901.2144 🔍 (source)
|
total cluster mass |
|
4000000000000000.0 M_\odot |
|
|
0901.2587 🔍 (source)
|
clustering length |
r _ { 0 } |
4.4 ± 0.12 Mpc h-1 |
|
|
0901.3943 🔍 (source)
|
cluster distance modulus |
|
9.63 ± 0.08 |
|
|
0901.4733 🔍 (source)
|
clustering radius |
r _ { 0 } |
5.3 ± 0.6 |
|
|
0902.0363 🔍 (source)
|
clustering scale length |
r _ { 0 } |
5.95 ± 0.9 Mpc h-1 |
|
|
0902.1098 🔍 (source)
|
clustering amplitude |
s _ { o } |
6.4 ± 0.8 Mpc h-1 |
|
|
0902.4027 🔍 (source)
|
cluster mass |
|
14000000.0 +4000000.0-5000000.0 M_\odot |
|
|
0902.4040 🔍 (source)
|
cluster average radial velocity |
|
2.34 ± 0.05 km s-1 |
|
|
0903.4911 🔍 (source)
|
cluster star-formation rate |
{ SFR } _ { 24 \mu { m } } { |
910.0 ± 320.0 M_\odot yr-1 |
|
|
0904.2392 🔍 (source)
|
cluster exponent |
\alpha |
0.37 |
|
|
0904.2392 🔍 (source)
|
cluster exponent |
\alpha |
0.5 |
|
|
0904.3342 🔍 (source)
|
median cluster radius |
|
0.7 pc |
|
|
0904.3329 🔍 (source)
|
mean cluster velocity |
\langle v _ { r } \rangle |
-20.3 ± 0.7 km s-1 |
|
|
0904.4701 🔍 (source)
|
cluster distance modulus |
|
15.46 ± 0.11 mag |
|
|
0905.1889 🔍 (source)
|
characteristic cluster tidal radius |
|
10.0 pc |
|
|
0905.2427 🔍 (source)
|
integral upper limit to the VHE energy emission of the globular cluster M13 |
F ( E > 200 ~ { } \textrm { GeV } ) |
5.1e-12 cm-2 s-1 |
Upper |
|
0906.2006 🔍 (source)
|
cluster radial velocities |
v _ { \scriptsize R } |
-160.0 |
Lower |
|
0907.4232 🔍 (source)
|
cluster redshift |
r _ { e } |
140.0 kpc |
|
|
0907.4232 🔍 (source)
|
cluster redshift |
z _ { |
140.0 kpc |
|
|
0908.3003 🔍 (source)
|
rms cluster-to-cluster scatter |
|
0.03 |
|
|
0909.3267 🔍 (source)
|
cluster core region |
|
8.0 |
Upper |
|
0909.3303 🔍 (source)
|
mean level of the cluster horizontal |
\langle V ( RR ) \rangle |
25.18 ± 0.02 |
|
|
0909.5154 🔍 (source)
|
total cluster dust mass-loss rate |
|
3.0000000000000004e-09 +2e-09-1.2e-09 M_\odot yr-1 |
|
|
0910.1732 🔍 (source)
|
cluster radii |
|
1.075 ± 0.8049999999999999 pc |
|
|
0910.1732 🔍 (source)
|
cluster radii |
|
6.734999999999999 +4.535-4.534999999999999 pc |
|
|
0910.5110 🔍 (source)
|
metallicity clusters |
O/H ] |
-0.7 dex |
|
|
0911.2339 🔍 (source)
|
temperature of the cluster gas decreases |
|
9.0 ± 0.5 keV |
|
|
0911.2339 🔍 (source)
|
temperature of the cluster gas decreases |
|
1.3 ± 0.2 keV |
|
|
0911.4925 🔍 (source)
|
Supercluster |
l |
275.0 |
|
|
0911.4925 🔍 (source)
|
Supercluster |
|
3500.0 |
|
|
0911.4925 🔍 (source)
|
Supercluster |
|
-1.0 |
|
|
0911.4925 🔍 (source)
|
Supercluster |
|
56.0 Mpc |
|
|
0912.0039 🔍 (source)
|
total cluster flux |
|
2e-15 erg cm-2 s-1 |
|
|
0912.0321 🔍 (source)
|
cluster age |
|
0.14 ± 0.03 |
|
|
0912.2061 🔍 (source)
|
total cluster mass |
|
1600.0 ± 400.0 M_\odot |
|
|
0912.4730 🔍 (source)
|
cluster masses |
|
0.1 |
|
|
1002.5037 🔍 (source)
|
cluster total mass ratio |
M _ { \bullet } / M |
0.0058 +0.0009000000000000001-0.0012 |
|
|
1002.5037 🔍 (source)
|
cluster total mass |
M |
3100000.0 ± 300000.0 M_\odot |
|
|
1003.0680 🔍 (source)
|
total nuclear star cluster mass |
|
11000000.0 M_\odot |
|
|
1003.1521 🔍 (source)
|
fraction of cluster SNe |
|
9.4 +8.3-5.1 |
|
|
1003.2208 🔍 (source)
|
cluster |
|
4300.0 +3300.0-1500.0 M_\odot |
|
|
1004.3738 🔍 (source)
|
mean radial velocity of the cluster |
\overline { RV _ { cl } } \pm \overline { \sigma _ { cl } } ) |
-29.11 ± 0.85 km s-1 |
|
|
1005.3028 🔍 (source)
|
clustering scale-length |
r _ { 0 } |
3.19 +0.32-0.54 Mpc h-1 |
|
|
1005.3619 🔍 (source)
|
mean Pleiades cluster metallicity |
[ Fe / H ] |
0.01 ± 0.02 |
|
|
1005.4699 🔍 (source)
|
cluster peculiar velocity |
v _ { z } |
-226.0 ± 275.0 km s-1 |
|
|
1006.3757 🔍 (source)
|
cluster SN rate |
|
0.35 |
|
|
1006.5121 🔍 (source)
|
peak height of the cluster |
\nu |
5.6 |
|
|
1006.5217 🔍 (source)
|
cluster age |
|
11.0 ± 1.5 Gyr |
|
|
1006.5217 🔍 (source)
|
cluster age |
|
11.0 ± 1.5 Gyr |
|
|
1006.5217 🔍 (source)
|
cluster age |
|
10.0 ± 1.5 Gyr |
|
|
1006.5654 🔍 (source)
|
cluster distance |
|
741.0 ± 36.0 pc |
|
|
1006.5654 🔍 (source)
|
average cluster reddening |
E ( B - V ) |
0.37 ± 0.05 mag |
|
|
1009.0920 🔍 (source)
|
cluster distance |
|
3.6 ± 0.2 kpc |
|
|
1009.3930 🔍 (source)
|
total cluster mass |
M _ { 200 } ^ { tot } |
455999999999999.94 ± 229999999999999.97 M_\odot |
|
|
1010.0469 🔍 (source)
|
mean heliocentric radial velocity of the cluster |
|
31.5 ± 0.4 km s-1 |
|
|
1010.5786 🔍 (source)
|
single-burst cluster formation redshift |
z _ { f } |
3.0 |
|
|
1010.5786 🔍 (source)
|
fraction of stars in the intra-cluster medium |
|
0.47 |
Upper |
|
1011.1310 🔍 (source)
|
intracluster stellar mass fraction |
|
0.16 +0.13-0.09 |
|
|
1011.1310 🔍 (source)
|
intracluster stellar mass fraction |
|
0.47 |
Upper |
|
1012.4996 🔍 (source)
|
mean cluster total mass |
M _ { T } ( r _ { 200 } ) |
590000000000000.0 ± 340000000000000.0 M_\odot |
|
|
1101.0813 🔍 (source)
|
cluster mass function index |
\beta _ { \star } |
2.0 |
|
|
1102.1837 🔍 (source)
|
cluster mass |
M _ { vir } |
750000000000000.0 +270000000000000.03-190000000000000.0 M_\odot |
|
|
1103.0785 🔍 (source)
|
cluster age |
|
7.5 ± 2.5 Myr |
|
|
1103.4144 🔍 (source)
|
cluster reddening |
E ( B - V ) |
0.22 ± 0.02 |
|
|
1106.1376 🔍 (source)
|
cluster mass |
M _ { 500 } |
780000000000000.0 ± 80000000000000.0 M_\odot |
|
|
1106.5784 🔍 (source)
|
cluster mass |
M _ { 200 } |
120000000000000.0 M_\odot |
|
|
1108.3567 🔍 (source)
|
mean cluster reddening |
E _ { B - V } |
1.45 ± 0.07 |
|
|
1109.0314 🔍 (source)
|
total cluster masses |
|
3000.0 ± 800.0 |
|
|
1109.0314 🔍 (source)
|
total cluster masses |
|
8000.0 ± 1500.0 |
|
|
1109.0953 🔍 (source)
|
cluster mass |
M _ { 200 a } |
2160000000000000.2 ± 320000000000000.0 h |
|
|
1110.6446 🔍 (source)
|
cluster-centric distance |
M |
134000000000.00002 M_\odot |
Lower |
|
1111.0992 🔍 (source)
|
cluster radius |
|
0.55 +0.44999999999999996-0.45000000000000007 |
|
|
1111.2630 🔍 (source)
|
cluster age |
|
3.7 +0.4-0.5 Myr |
|
|
1112.5458 🔍 (source)
|
bulk motion of the Arches cluster |
|
172.0 ± 15.0 km s-1 |
|
|
1112.5458 🔍 (source)
|
total cluster mass |
M _ { cl } |
50000.0 ± 10000.0 M_\odot |
|
|
1112.5458 🔍 (source)
|
total present-day mass of the cluster |
M ( r < 1.0 ~ { } { pc } ) |
15000.0 +7400.0-6000.0 M_\odot |
|
|
1201.5395 🔍 (source)
|
total cluster luminosity |
L _ { X } |
2e+44 |
|
|
1202.4461 🔍 (source)
|
cluster |
|
1.7 ± 0.4 % |
|
|
1203.1326 🔍 (source)
|
eight protocluster |
|
647.0 ± 124.0 km s-1 |
|
|
1203.5337 🔍 (source)
|
average number of detected excess AGN per cluster environment |
|
3.0 ± 0.7 |
|
|
1203.5337 🔍 (source)
|
average number of detected excess AGN per cluster environment |
|
3.5 ± 0.9 |
|
|
1204.3635 🔍 (source)
|
clustering scale lengths |
|
3.46 ± 0.41 |
|
|
1204.3635 🔍 (source)
|
clustering scale lengths |
r _ { 0 } |
3.83 ± 0.24 Mpc h-1 |
|
|
1204.5759 🔍 (source)
|
intracluster plasma |
L _ { mech } |
44.5 ± 0.5 |
Upper |
|
1204.6316 🔍 (source)
|
cluster impact parameter range |
|
1.005 +0.645-0.6449999999999999 Mpc (0.23 - 1.05 R _ vir) |
|
|
1205.2693 🔍 (source)
|
mean cluster velocity |
|
72.55 ± 0.22 km s-1 |
|
|
1205.2693 🔍 (source)
|
total cluster mass |
|
29.0 |
|
|
1206.4052 🔍 (source)
|
clustering amplitude equivalent to a correlation length |
r _ { 0 } |
3.7 ± 0.3 Mpc h-1 |
|
|
1206.4552 🔍 (source)
|
fraction of the candidate cluster members |
|
81.0 % |
|
|
1207.3793 🔍 (source)
|
clustercentric radius |
|
30.0 kpc (2.9 \pm 0.4 \times 10 ^ 9 M _ \odot) |
|
|
1207.6235 🔍 (source)
|
north-western cluster component |
M ( { < } 75 { kpc } ) |
56000000000000.0 ± 5000000000000.0 M_\odot |
|
|
1207.6235 🔍 (source)
|
north-western cluster component |
|
22500000000000.0 ± 7500000000000.0 M_\odot |
|
|
1207.7301 🔍 (source)
|
mean cluster age |
|
7.0 ± 1.3 Gyr |
|
|
1207.7301 🔍 (source)
|
mean cluster metallicity |
[ Fe / H ] |
-1.0 ± 0.15 dex |
|
|
1208.0667 🔍 (source)
|
cluster recession velocity |
|
21257.0 ± 54.0 km s-1 |
|
|
1208.6419 🔍 (source)
|
mass of young clusters |
|
2.0 |
Upper |
|
1209.3910 🔍 (source)
|
cluster radius |
|
2.85 ± 0.5 pc |
|
|
1209.6460 🔍 (source)
|
clustering length |
r _ { 0 } |
7.2 ± 0.6 Mpc h-1 |
|
|
1210.5927 🔍 (source)
|
average cluster redshift |
z \right |
0.322 |
Lower |
|
1210.7242 🔍 (source)
|
cluster metallicity |
Fe / H ] _ { ZW } |
-1.63 ± 0.14 |
|
|
1212.5460 🔍 (source)
|
typical cluster size |
|
0.3 ± 0.05 kpc |
|
|
1301.0540 🔍 (source)
|
cluster |
\alpha |
1.7 ± 0.2 |
|
|
1301.0540 🔍 (source)
|
cluster |
|
4.15 +1.6499999999999995-1.6500000000000004 Myr |
|
|
1301.0540 🔍 (source)
|
cluster |
|
3.9 Myr |
|
|
1301.5200 🔍 (source)
|
mean cluster redshift |
z \right |
0.168 |
Lower |
|
1302.3754 🔍 (source)
|
typical cluster size |
|
0.3 ± 0.05 kpc |
|
|
1302.4754 🔍 (source)
|
dark matter clustering strength |
F _ { cl } |
0.99 ± 0.02 |
|
|
1302.6253 🔍 (source)
|
cluster AGN fraction |
f _ { A } |
3.0 +2.4-1.4 % |
|
|
1303.2847 🔍 (source)
|
mean cluster redshift |
|
0.06228 ± 0.00015 |
|
|
1303.2847 🔍 (source)
|
cluster electron density |
n _ { e , 0 } |
0.0010600000000000002 ± 0.00011 cm-3 |
|
|
1305.3606 🔍 (source)
|
cluster metallicity |
Fe / H ] _ { ZW } |
-2.01 ± 0.04 |
|
|
1306.5579 🔍 (source)
|
cluster luminosity |
L _ { ( 0.5 - 2 keV ) } |
3.0000000000000003e+44 erg s-1 |
|
|
1306.5579 🔍 (source)
|
cluster |
kT |
4.4 +0.5-0.3 keV |
|
|
1306.6339 🔍 (source)
|
cluster age |
|
22.0 ± 4.0 Myr |
|
|
1306.6496 🔍 (source)
|
galaxy cluster velocity dispersion |
\sigma _ { gal } / \sigma _ { DM } |
0.9099999999999999 +0.040000000000000036-0.039999999999999925 |
|
|
1307.2020 🔍 (source)
|
total cluster mass |
|
630.0 M_\odot |
|
|
1307.6217 🔍 (source)
|
cluster distance |
|
5.2 kpc |
|
|
1308.2761 🔍 (source)
|
buildup of the nuclear bar and nuclear star cluster |
R |
30.0 pc |
Upper |
|
1309.2587 🔍 (source)
|
cluster center |
|
2.3 |
Lower |
|
1310.2178 🔍 (source)
|
cluster radius |
|
3.2 ± 0.2 pc |
|
|
1310.2612 🔍 (source)
|
cluster dissolution fraction |
|
88.0 ± 8.0 |
|
|
1310.5621 🔍 (source)
|
cluster formation efficiency |
\Gamma |
33.0 % |
|
|
1312.1694 🔍 (source)
|
total cluster SFR enclosed |
|
1161.0 ± 96.0 M_\odot yr-1 |
|
|
1312.4593 🔍 (source)
|
clustering signal of absorbers on projected scales |
r _ { p } |
17.65 +17.35-17.349999999999998 Mpc h-1 |
|
|
1312.5982 🔍 (source)
|
cluster masses |
|
170000.0 |
|
|
1312.5982 🔍 (source)
|
cluster masses |
|
140000.0 |
|
|
1312.5982 🔍 (source)
|
cluster masses |
|
110000.00000000001 M_\odot |
|
|
1401.1563 🔍 (source)
|
cluster age |
|
1.5 +0.2-0.1 Gyr |
|
|
1403.1705 🔍 (source)
|
cluster-centric radius |
|
16.0 +11.0-8.0 c-1 |
|
|
1403.2741 🔍 (source)
|
median subcluster ages range |
|
0.5 Myr |
|
|
1403.2741 🔍 (source)
|
median subcluster ages range |
|
5.0 Myr |
|
|
1403.3168 🔍 (source)
|
concentration of cluster X-ray morphology |
Spearman \rho |
-0.79 |
|
|
1403.3428 🔍 (source)
|
cluster total mass |
|
2800.0 +1600.0-1400.0 M_\odot |
|
|
1404.0023 🔍 (source)
|
spatial clustering correlation scale length |
r _ { 0 } |
32.0 ± 7.0 Mpc h-1 |
|
|
1405.0496 🔍 (source)
|
protocluster dynamical mass |
|
410.0 ± 260.0 M_\odot |
|
|
1405.3662 🔍 (source)
|
numbers of globular clusters and dwarf satellites |
M _ { M 31 } / M _ { MW } |
1.0 |
Lower |
|
1405.4707 🔍 (source)
|
cluster mass |
|
2500000000000000.0 ± 1500000000000000.0 h |
|
|
1405.5881 🔍 (source)
|
cluster formation efficiency |
\Gamma |
7.0 ± 2.0 % |
|
|
1405.6586 🔍 (source)
|
cluster |
[ Fe / H ] |
-0.057 ± 0.018 dex |
|
|
1406.6703 🔍 (source)
|
cluster mass |
|
2000000000000000.0 M_\odot |
|
|
1407.5859 🔍 (source)
|
cluster age |
|
1.6 ± 0.1 Gyr |
|
|
1408.2821 🔍 (source)
|
GC-to-total cluster mass formation efficiency |
\epsilon _ { t } |
2.9e-05 ± 5e-06 |
|
|
1408.2821 🔍 (source)
|
cluster-wide specific frequency |
S _ { N , CL } |
2.8 ± 0.7 |
|
|
1408.3117 🔍 (source)
|
cluster ’ s radial-velocity dispersion |
\sigma _ { c } |
0.62 ± 0.1 km s-1 |
|
|
1411.3677 🔍 (source)
|
cluster |
q _ { FIR } |
1.8 ± 0.15 |
|
|
1411.5688 🔍 (source)
|
clustering length |
r _ { 0 } |
3.95 +0.48-0.54 Mpc h-1 |
|
|
1412.6717 🔍 (source)
|
fraction of cluster ETGs |
SFR |
26.0 M_\odot yr-1 |
Lower |
|
1501.01215 🔍 (source)
|
clustering length |
r _ { 0 } |
3.29 ± 0.57 Mpc h-1 |
|
|
1501.01215 🔍 (source)
|
clustering length |
r _ { 0 } |
2.86 ± 0.33 Mpc h-1 |
|
|
1502.02102 🔍 (source)
|
total cluster mass |
|
78.0 ± 18.0 M_\odot |
|
|
1502.05088 🔍 (source)
|
subclusters ’ gas temperatures |
|
2.5 ± 0.5 keV |
|
|
1502.07345 🔍 (source)
|
cluster |
|
-2.07 ± 0.06 |
|
|
1502.07345 🔍 (source)
|
cluster |
[ Fe / H ] |
-2.2 ± 0.1 |
|
|
1503.03372 🔍 (source)
|
young clusters |
|
10.0 Myr |
Upper |
|
1503.05676 🔍 (source)
|
cluster average metallicity |
|
-0.08 ± 0.06 |
|
|
1505.02869 🔍 (source)
|
cluster radii |
|
1.1 ± 0.63 |
|
|
1505.02869 🔍 (source)
|
cluster radii |
|
5.36 ± 0.24 |
|
|
1505.03407 🔍 (source)
|
galaxy cluster luminosity function |
\alpha _ { d } |
-1.5 |
|
|
1505.05653 🔍 (source)
|
clustering strength |
r _ { 0 } |
15.0 ± 2.5 Mpc |
|
|
1505.07475 🔍 (source)
|
cluster population ( slope |
|
-2.18 ± 0.07 |
|
|
1505.07233 🔍 (source)
|
total estimated mass of the supercluster |
M _ { est } |
6200000000000000.0 M_\odot |
|
|
1505.07504 🔍 (source)
|
cluster rotation |
|
0.024 ± 0.013 km s-1 |
|
|
1507.02285 🔍 (source)
|
Intra-Cluster Medium ( ICM ) temperature |
|
8.5 +0.8-0.6 keV |
Lower |
|
1507.02285 🔍 (source)
|
Intra-Cluster Medium ( ICM ) temperature |
|
2.7 +0.7-0.4 keV |
|
|
1507.02687 🔍 (source)
|
clustering length |
r _ { 0 } |
3.3 ± 0.8 Mpc h-1 |
|
|
1508.04894 🔍 (source)
|
distance modulus of the cluster |
|
14.74 ± 0.04 mag |
|
|
1508.04894 🔍 (source)
|
age of the cluster |
|
12.5 ± 0.5 Gyr |
|
|
1508.07394 🔍 (source)
|
emission radii of kHz QPOs cluster |
|
17.5 ± 1.5 km |
|
|
1509.00219 🔍 (source)
|
clustering length |
r _ { 0 } |
6.21 ± 0.78 |
|
|
1510.00718 🔍 (source)
|
metallicity of both the intracluster medium |
M _ { vir } |
600000000000000.0 M_\odot h-1 |
|
|
1510.05385 🔍 (source)
|
mean cluster metallicity |
\mathrm { [ Fe / H ] |
0.07 ± 0.03 dex |
|
|
1510.05951 🔍 (source)
|
X-ray temperature of the hot intracluster medium |
kT |
5.3 ± 0.3 keV |
|
|
1511.01118 🔍 (source)
|
cluster masses |
|
165.0 |
|
|
1511.01118 🔍 (source)
|
cluster masses |
M _ { cl } |
50.0 |
Upper |
|
1511.01907 🔍 (source)
|
age of the host cluster |
|
165.0 ± 135.0 Myr |
|
|
1511.03731 🔍 (source)
|
massive galaxy cluster |
M _ { 200 } ^ { crit } |
1100000000000000.1 M_\odot h-1 |
|
|
1511.06354 🔍 (source)
|
cluster distance |
|
8.5 ± 1.0 kpc |
|
|
1511.08493 🔍 (source)
|
total number of clusters |
N _ { GC } |
39000.0 ± 2000.0 |
|
|
1512.02095 🔍 (source)
|
bulk of the cluster population |
|
0.35 +0.25-0.24999999999999997 M_\odot |
|
|
1512.04983 🔍 (source)
|
average cluster radial velocity |
|
-42.36 ± 0.04 km s-1 |
|
|
1601.00682 🔍 (source)
|
SFR of the protocluster AGNs |
|
160.0 ± 50.0 M_\odot yr-1 |
|
|
1601.02186 🔍 (source)
|
total cluster mass |
|
352.0 M_\odot |
|
|
1602.02503 🔍 (source)
|
A cluster age |
|
4.0 ± 0.8 Myr |
|
|
1602.08598 🔍 (source)
|
clustering comoving length |
x _ { 0 } |
5.4 ± 1.0 Mpc h-1 |
|
|
1602.08598 🔍 (source)
|
s inverted spatial comoving clustering length |
x _ { 0 } |
5.5 ± 1.2 Mpc h-1 |
|
|
1603.03904 🔍 (source)
|
average central optical depth of the cluster |
\bar { \tau } _ { e } |
0.00375 ± 0.0008900000000000001 |
|
|
1603.04994 🔍 (source)
|
cluster age |
|
1.5 +0.3-0.7 Myr |
|
|
1603.08072 🔍 (source)
|
clustering bias of BH binaries |
b _ { BH , 0 } |
1.5 |
Lower |
|
1604.00144 🔍 (source)
|
disk fraction of the cluster |
|
27.0 ± 6.0 % |
|
|
1604.00144 🔍 (source)
|
cluster members |
A _ { V } |
14.5 ± 10.5 mag |
|
|
1604.07871 🔍 (source)
|
clustering amplitude of the matter power spectrum |
\sigma _ { 8 } |
0.74 ± 0.13 |
|
|
1605.02822 🔍 (source)
|
clustering fraction |
|
30.0 |
|
|
1605.05314 🔍 (source)
|
SFR of cluster star-forming galaxies |
|
2.0 |
Lower |
|
1606.03015 🔍 (source)
|
mean cluster parallax |
|
7.42 ± 0.09 m as |
|
|
1606.03015 🔍 (source)
|
mean cluster distance |
|
134.8 ± 1.7 pc |
|
|
1606.05016 🔍 (source)
|
intra-cluster medium temperatures |
|
3.0 ± 2.0 keV |
|
|
1606.06425 🔍 (source)
|
average cluster scale height |
|
60.0 ± 2.0 pc |
|
|
1606.06425 🔍 (source)
|
average cluster scale height |
z _ { h } |
64.0 ± 2.0 pc |
|
|
1606.08286 🔍 (source)
|
clustering |
r _ { 0 } |
11.7 +1.0-1.1 Mpc |
|
|
1606.08286 🔍 (source)
|
clustering |
r _ { 0 } |
11.2 +2.5-3.3 Mpc |
|
|
1606.08608 🔍 (source)
|
cluster |
\mu _ { V } |
9.3 ± 0.07 mag |
|
|
1606.08608 🔍 (source)
|
cluster |
V _ { r } |
-8.3 ± 5.0 km s-1 |
|
|
1607.01617 🔍 (source)
|
cluster Ia rate |
|
0.14 +0.19-0.09 ± 0.01 S N |
|
|
1607.06102 🔍 (source)
|
mean cluster abundance |
[ Fe / H ] |
-0.16 ± 0.04 |
|
|
1608.06289 🔍 (source)
|
projected cluster-centric distance |
|
-0.15 ± 0.08 dex Mpc-1 |
|
|
1609.04509 🔍 (source)
|
cluster metallicity |
M/H ] |
-1.6 ± 0.2 |
|
|
1610.00637 🔍 (source)
|
hot imprint of superclusters |
\Delta T _ { f } |
5.1 ± 3.2 K |
|
|
1610.01498 🔍 (source)
|
sSFR of the entire cluster population declines |
|
0.48 ± 0.06 Gyr-1 |
Lower |
|
1610.01498 🔍 (source)
|
sSFR of the entire cluster population declines |
|
0.043 ± 0.009 Gyr-1 |
Upper |
|
1610.01498 🔍 (source)
|
fraction of quiescent cluster galaxies |
|
28.0 +8.0-19.0 |
|
|
1610.09144 🔍 (source)
|
clustering length |
s _ { 0 } |
0.081 ± 0.006 Mpc h-1 |
|
|
1610.09144 🔍 (source)
|
cross-clustering length |
s _ { 0 } |
0.27 ± 0.14 Mpc h-1 |
|
|
1610.09144 🔍 (source)
|
real-space clustering length |
r _ { 0 } |
0.24 ± 0.04 Mpc h-1 |
|
|
1611.00835 🔍 (source)
|
ages of these clusters |
|
1.35 ± 0.05 |
|
|
1611.00835 🔍 (source)
|
ages of these clusters |
|
1.02 ± 0.02 |
|
|
1611.00835 🔍 (source)
|
ages of these clusters |
|
1.64 ± 0.04 |
|
|
1611.00835 🔍 (source)
|
ages of these clusters |
|
0.86 ± 0.04 Gyr |
|
|
1611.05816 🔍 (source)
|
average galaxy cluster velocity anisotropy parameter |
\beta |
0.248 +0.164-0.36 |
|
|
1612.04395 🔍 (source)
|
cluster distance |
|
5.9 kpc |
|
|
1612.05181 🔍 (source)
|
cluster distance |
|
4.4 ± 0.4 kpc |
|
|
1701.07302 🔍 (source)
|
total stellar cluster mass |
|
36000.0 ± 3000.0 M_\odot |
|
|
1702.03491 🔍 (source)
|
small-scale quasar clustering amplitude |
|
24.1 ± 3.6 |
|
|
1702.03491 🔍 (source)
|
small-scale quasar clustering amplitude |
A |
26.6 kpc h-1 |
|
|
1702.03933 🔍 (source)
|
ratio of the clustering amplitudes |
w _ { red } / w _ { blue } |
1.92 ± 0.11 |
|
|
1703.02033 🔍 (source)
|
cluster |
RA _ { J 2000 } |
16.0 |
|
|
1703.02033 🔍 (source)
|
cluster |
\langle P \rangle |
0.54 day |
|
|
1703.02033 🔍 (source)
|
cluster |
[ Fe / H ] |
-1.5 ± 0.4 dex |
|
|
1703.02033 🔍 (source)
|
cluster |
A _ { K _ { s } } |
0.38 ± 0.02 |
|
|
1703.02616 🔍 (source)
|
mean redshift of the cluster core |
|
0.0594 ± 0.0005 |
|
|
1703.04803 🔍 (source)
|
two subclusters |
|
924.0 +243.0-206.0 kpc |
|
|
1703.04803 🔍 (source)
|
two subclusters |
|
92.0 ± 164.0 km s-1 |
|
|
1703.08444 🔍 (source)
|
superclusters |
|
0.2 |
Upper |
|
1703.08444 🔍 (source)
|
superclusters |
|
-80000000000000.0 L_\odot h-2 |
|
|
1705.03370 🔍 (source)
|
age distribution of clusters declines |
dN / d \tau |
-0.3 |
Upper |
|
1706.00427 🔍 (source)
|
total cluster mass |
|
13.0 ± 4.0 |
|
|
1706.01366 🔍 (source)
|
systemic redshift of the cluster galaxies |
z |
1.709 |
|
|
1706.01961 🔍 (source)
|
cluster radius |
r _ { cl } |
0.0 |
|
|
1708.06875 🔍 (source)
|
total cluster mass |
|
6800.0 ± 3400.0 M_\odot |
|
|
1709.02809 🔍 (source)
|
total obscured SFR of the proto-cluster could rise |
|
14.0 |
|
|
1709.04945 🔍 (source)
|
average mass per cluster |
|
220000000000000.03 M_\odot |
|
|
1709.04945 🔍 (source)
|
average mass per cluster |
|
19.0 ± 5.0 % |
|
|
1710.10666 🔍 (source)
|
distance to the cluster kinematically |
|
4.29 ± 0.47 kpc |
|
|
1711.00475 🔍 (source)
|
cluster mass |
M _ { 200 c } / ( 10 ^ { 15 } M _ { \odot } ) |
2.06 +0.28-0.26 (% stat) ± 0.12 (sys) |
|
|
1711.06043 🔍 (source)
|
cluster age |
|
3.0 Myr |
Upper |
|
1711.07806 🔍 (source)
|
clustercentric distances |
D _ { \mathrm { c } |
1.8 h-1 |
|
|
1711.09500 🔍 (source)
|
total globular cluster population |
N _ { tot } |
3441.0 ± 1416.0 |
|
|
1801.01140 🔍 (source)
|
intracluster light ( ICL ) fraction |
|
7.21 ± 1.53 % |
|
|
1801.03015 🔍 (source)
|
sub-cluster ICM temperatures |
|
5.17 +0.2-0.19 keV |
|
|
1801.03584 🔍 (source)
|
cluster transverse velocities |
v _ { T } |
1000.0 km s-1 |
Upper |
|
1802.06779 🔍 (source)
|
fraction of older clusters |
t |
1.0 |
Lower |
|
1802.08270 🔍 (source)
|
metallicity cluster |
[ M / H ] |
0.4 |
|
|
1803.02927 🔍 (source)
|
absolute cluster age |
|
13.4 ± 0.7 ± 1.2 Gyr |
|
|
1804.00635 🔍 (source)
|
peak of the cluster age distribution |
|
130.0 ± 35.0 Myr |
|
|
1807.02794 🔍 (source)
|
age of the cluster |
|
677.5 ± 97.5 Myr |
|
|
1807.10612 🔍 (source)
|
dynamical cluster mass |
|
140000.0 ± 20000.0 M_\odot |
|
|
1808.01726 🔍 (source)
|
star cluster formation efficiency |
\epsilon _ { max } |
0.9 |
Upper |
|
1808.02577 🔍 (source)
|
cluster radii |
|
0.25 pc |
|
|
1808.02577 🔍 (source)
|
cluster radii |
|
3.0 pc |
|
|
1808.02204 🔍 (source)
|
radii of young star clusters in the local universe |
r _ { v } |
2.75 ± 2.25 pc |
|
|
1809.06868 🔍 (source)
|
cluster average |
[ Fe / H ] |
0.08 |
|
|
1810.02388 🔍 (source)
|
weighted average distance to the cluster |
|
5.4 ± 0.1 kpc |
|
|
1810.03633 🔍 (source)
|
age of the stellar cluster |
|
5.5 Myr |
|
|
1810.09897 🔍 (source)
|
cluster formation efficiency |
\Gamma |
19.0 c-1 |
|
|
1810.12071 🔍 (source)
|
cluster mass |
M _ { 200 } |
1150000000000000.0 +300000000000000.0-350000000000000.0 M_\odot |
|
|
1811.00556 🔍 (source)
|
clustering lengths |
r _ { 0 } |
4.5 ± 1.5 Mpc h-1 |
|
|
1812.06926 🔍 (source)
|
intrinsic cluster-to-cluster scatter |
\sigma _ { \footnotesize int } |
470.0 ± 340.0 km s-1 |
|
|
1901.03711 🔍 (source)
|
average velocity of the globular clusters |
\langle v _ { gc } \rangle |
1803.0 ± 2.0 km s-1 |
|
|
1901.11375 🔍 (source)
|
cluster distance |
|
1915.0 ± 110.0 pc |
|
|
1903.02579 🔍 (source)
|
cluster |
\mu / Gyr ^ { -1 } |
1.0 |
Upper |
|
1904.02280 🔍 (source)
|
cluster distance |
|
1847.0 ± 107.0 pc |
|
|
1905.00914 🔍 (source)
|
cluster redshift |
z _ { c } |
0.972 |
|
|
1906.08550 🔍 (source)
|
average cluster abundance |
\langle [ Fe / H ] \rangle |
-1.8 ± 0.03 |
|
|
1907.02357 🔍 (source)
|
cluster ’ s spectrophotometric distance |
|
10.2 ± 1.6 kpc |
|
|
1911.03477 🔍 (source)
|
total cluster mass |
|
88000.0 +17000.0-18000.0 M_\odot |
|
|
1911.05093 🔍 (source)
|
cluster formation efficiency |
\Gamma |
20.0 |
|
|
1912.00075 🔍 (source)
|
fraction of cluster galaxies hosting |
|
1.0 ± 0.4 |
|
|
2001.00506 🔍 (source)
|
temperature of the hot cluster medium |
|
3.9 keV |
|
|
2001.01481 🔍 (source)
|
age of the cluster |
|
12.0 ± 0.5 Gyr |
|
|
2001.03179 🔍 (source)
|
clusters |
\tau |
150.0 Myr |
Upper |
|
2001.04068 🔍 (source)
|
mean cluster parallax |
|
0.86 ± 0.05 m as |
|
|
2001.04068 🔍 (source)
|
cluster |
E ( B - V ) |
0.24 ± 0.02 mag |
|
|
2001.07398 🔍 (source)
|
cluster |
|
-0.88 ± 0.14 m as yr-1 |
|
|
2001.07398 🔍 (source)
|
cluster |
|
3.84 ± 0.15 kpc |
|
|
2001.07398 🔍 (source)
|
cluster |
|
0.8 ± 0.2 mag |
|
|
2003.09325 🔍 (source)
|
precise cluster age |
|
20.0 +3.5-2.6 Myr |
|
|
2004.06812 🔍 (source)
|
cluster binary fraction |
|
11.0 % |
|
|
2005.02840 🔍 (source)
|
cluster formation rate |
|
300.0 Myr |
Upper |
|
2006.01690 🔍 (source)
|
present-day cluster-formation rate |
|
0.6 ± 0.1 Myr-1 kpc-2 |
|
|
2006.12501 🔍 (source)
|
cluster |
|
23.6 ± 0.2 kpc |
|
|
2006.12501 🔍 (source)
|
cluster |
L _ { V } |
5100.0 +9700.0-3400.0 L_\odot |
|
|
2006.12501 🔍 (source)
|
cluster |
|
75.0 Myr |
|
|
2006.13618 🔍 (source)
|
cluster radius |
|
7.75 |
|
|
2006.13618 🔍 (source)
|
cluster radius |
|
5.63 pc |
|
|
2007.06594 🔍 (source)
|
average age of the oldest globular clusters |
t _ { GC } |
13.13 +0.15-0.1 (stat) ± 0.5 (sys) |
|