|
astro-ph/9604119 🔍 (source)
|
blue fractions of the intermediate redshift |
f _ { b } |
0.25 ± 0.04999999999999999 |
|
|
astro-ph/9701068 🔍 (source)
|
two intermediate delays |
|
1.13 +0.18-0.17 |
|
|
astro-ph/9702204 🔍 (source)
|
intermediate |
age |
2.3 Gyr |
|
|
astro-ph/9903029 🔍 (source)
|
bulk of the intermediate-age population |
t |
1.35 +1.15-1.1500000000000001 Gyr |
|
|
astro-ph/0203389 🔍 (source)
|
intermediate-velocity |
v |
-220.0 km s-1 |
Upper |
|
astro-ph/0209165 🔍 (source)
|
intermediate-to-major axis ratio |
q _ { b } |
0.85 |
|
|
astro-ph/0210073 🔍 (source)
|
intermediate-age population |
|
200.0 Myr |
|
|
astro-ph/0305318 🔍 (source)
|
mass ) intermediate-age |
|
7.0 ± 1.0 |
|
|
astro-ph/0403136 🔍 (source)
|
intermediate-to-high metallicities |
[ Fe / H ] |
-1.3 |
Lower |
|
astro-ph/0410174 🔍 (source)
|
intermediate-age population |
\tau |
300.0 Myr |
|
|
astro-ph/0411775 🔍 (source)
|
SFR density of intermediate mass galaxies |
M _ { \star } |
10.8 M_\odot |
Upper |
|
astro-ph/0505104 🔍 (source)
|
number of young/intermediate age clusters |
|
2.0 Gyr |
|
|
astro-ph/0508285 🔍 (source)
|
Intermediate mass |
|
4.5 ± 3.5 M_\odot |
|
|
astro-ph/0512383 🔍 (source)
|
intermediate-age population |
|
300.0 Myr |
|
|
nucl-ex/0603005 🔍 (source)
|
Intermediate mass fragments |
|
27.0 A |
|
|
nucl-ex/0603005 🔍 (source)
|
Intermediate mass fragments |
|
59.0 C |
|
|
astro-ph/0609042 🔍 (source)
|
intermediate sizes |
r _ { 1 / 2 } |
6.0 ± 1.0 kpc |
|
|
0708.2847 🔍 (source)
|
life of intermediate |
|
25.0 M_\odot |
Upper |
|
0712.0725 🔍 (source)
|
metal abundance of intermediate mass |
|
3.45 ± 0.9500000000000002 M_\odot |
|
|
0801.1806 🔍 (source)
|
life of intermediate |
|
25.0 M_\odot |
Upper |
|
0803.1066 🔍 (source)
|
intermediate-age |
|
4.0 |
|
|
0804.2954 🔍 (source)
|
intermediate |
|
-0.7 |
Lower |
|
0903.1948 🔍 (source)
|
average of intermediate age |
|
1.5 ± 0.5 Gyr |
|
|
0907.5416 🔍 (source)
|
intermediate-to-low mass |
\log ( { \cal M } / { { \cal M } _ { \odot } } |
10.5 |
|
|
0909.1912 🔍 (source)
|
age of these intermediate-mass |
|
30.0 Myr |
Lower |
|
0911.1363 🔍 (source)
|
low–to–intermediate mass |
M _ { tot } |
0.2 M_\odot |
Lower |
|
1003.1132 🔍 (source)
|
intermediate/major axis ratio |
b / a ) _ { \Phi } |
0.99 |
|
|
1101.2869 🔍 (source)
|
intermediate age |
|
400000000.0 yr |
|
|
1111.4868 🔍 (source)
|
intermediate-age |
|
20.0 |
|
|
1201.4959 🔍 (source)
|
intermediate-high concentration |
c |
1.75 |
|
|
1211.3973 🔍 (source)
|
sizes of intermediate-mass |
\log ( M _ { \textrm { \scriptsize dyn } } / M _ { \odot } |
10.85 |
|
|
1310.1405 🔍 (source)
|
emergent flux of intermediate-separation |
|
20.0 |
|
|
1310.1405 🔍 (source)
|
emergent flux of intermediate-separation |
|
2.0 AU |
Upper |
|
1406.2747 🔍 (source)
|
intermediate-age |
|
7.15 ± 1.17 Gyr |
|
|
1509.00023 🔍 (source)
|
substantial intermediate-age population |
t |
3.0 Gyr |
|
|
1606.07809 🔍 (source)
|
mass fraction of intermediate-aged |
|
1.0 Gyr |
|
|
1612.01054 🔍 (source)
|
strength of the intermediate filaments |
|
96.0 ± 4.0 |
|
|
1804.00676 🔍 (source)
|
intermediate-to-major axis ratio |
q _ { b } |
0.63 |
Lower |
|
1811.01875 🔍 (source)
|
intermediate-age |
t |
50.0 Myr |
Lower |
|
1902.01557 🔍 (source)
|
incoming intermediate-duration gravitational |
|
4.4e-22 |
Upper |
|
1902.05571 🔍 (source)
|
total count of HTRU intermediate-latitude pulsars |
|
113.0 |
Upper |
|
1903.10918 🔍 (source)
|
six intermediate mass |
\log ( M _ { dyn } / M _ { \sun } |
9.7 |
|
|
2001.01839 🔍 (source)
|
massive intermediate age |
|
1.0 Gyr |
|