|
astro-ph/0101550 🔍 (source)
|
velocities relative |
|
62.5 ± 37.5 km s-1 |
Lower |
|
astro-ph/0105291 🔍 (source)
|
space velocity components relative |
U |
-9.8 ± 1.2 |
|
|
astro-ph/0208450 🔍 (source)
|
mean abundances relative to solar |
[ Si / H ] |
-1.26 ± 0.13 |
|
|
astro-ph/0305024 🔍 (source)
|
Oxygen abundances relative to hydrogen range |
Tree(positive_expression, [FunctionSymbol(LeafSymbol('log'), BinaryOperatorExpression('/', LeafSymbol('O'), LeafSymbol('H')))]) |
9.0 |
Upper |
|
astro-ph/0310346 🔍 (source)
|
Oxygen abundances relative to hydrogen range |
log ( O / H ) |
9.0 |
Upper |
|
astro-ph/0406513 🔍 (source)
|
amplitude of the linear redshift-space distortions relative to the galaxy overdensity field |
\beta ( L _ { * } , 0 ) |
0.58 ± 0.08 |
|
|
astro-ph/0504174 🔍 (source)
|
individual ^ { 16 } OH column densities relative to water give ratios |
[ H _ { 2 } O/OH |
0.8999999999999999 +0.30000000000000004-0.29999999999999993 |
|
|
astro-ph/0505141 🔍 (source)
|
Apparent speeds of jet components relative |
|
0.028 c |
Upper |
|
astro-ph/0506484 🔍 (source)
|
velocity dispersion of all nine stars relative |
|
15.0 ± 4.0 km s-1 |
|
|
astro-ph/0607376 🔍 (source)
|
metallicities relative to solar |
[ X / H ] |
-1.3 |
Lower |
|
0708.3088 🔍 (source)
|
CO abundances relative |
|
0.44 ± 0.03 % |
|
|
0801.3682 🔍 (source)
|
metallicities relative to solar |
[ X / H ] |
-1.3 |
Lower |
|
0804.0116 🔍 (source)
|
abundances relative |
|
-0.03 ± 0.12 |
|
|
0804.0116 🔍 (source)
|
abundances relative |
S |
0.16 ± 0.11 |
|
|
0908.0529 🔍 (source)
|
source-lens relative motion |
\mu |
5.0 m as yr-1 |
|
|
1001.4080 🔍 (source)
|
s relative |
\Delta \mu / \mu |
5.6e-06 ± 5.5e-06 (stat) ± 2.7e-06 (sys) |
|
|
1105.3108 🔍 (source)
|
kinetic temperature of this relatively warm gas |
T _ { kin } |
260.0 ± 240.0 K |
|
|
1301.4024 🔍 (source)
|
mass density of dust grains relative to hydrogen |
\rho _ { dust } / \rho _ { H } |
120.0 |
Lower |
|
1308.2470 🔍 (source)
|
gravitational potentials relative |
\Delta \phi |
0.1 |
|
|
1309.1371 🔍 (source)
|
proportion of dust mass relative to stellar mass |
M _ { dust } / M _ { star } |
0.02 % |
|
|
1310.6231 🔍 (source)
|
OH } abundances relative to total number of hydrogen atoms |
|
2.2999999999999998e-10 |
|
|
1401.1104 🔍 (source)
|
CH _ { 3 } OH abundances relative |
|
2.7 ± 0.3 % |
|
|
1401.1104 🔍 (source)
|
CH _ { 3 } OH abundances relative |
|
3.4 ± 0.6 % |
|
|
1410.7060 🔍 (source)
|
radial velocities relative |
|
-4.0 km s-1 |
|
|
1506.07878 🔍 (source)
|
s relative flux |
|
2.7 day |
|
|
1604.03939 🔍 (source)
|
ISW effect signal amplitudes relative |
A |
1.0 |
|
|
1609.07252 🔍 (source)
|
OCS abundances relative |
|
32.0 |
|
|
1701.03112 🔍 (source)
|
average strengths of these lines relative to the far-IR continuum |
|
0.00035999999999999997 ± 0.00012 |
|
|
1701.03112 🔍 (source)
|
average strengths of these lines relative to the far-IR continuum |
|
0.00084 ± 0.00017 |
|
|
1701.03112 🔍 (source)
|
average strengths of these lines relative to the far-IR continuum |
|
0.00027 ± 0.0001 |
|
|
1703.05491 🔍 (source)
|
mass fraction of baryons relative to the total dark matter halo |
m _ { d } |
0.05 |
Lower |
|
1703.08381 🔍 (source)
|
efficiency of transformation into dSphs relative to their |
f _ { gas } |
0.0 |
|
|
1707.06003 🔍 (source)
|
peak o- \mathrm { H } _ { 2 } S abundances relative |
|
4e-07 |
Lower |
|
1707.06003 🔍 (source)
|
peak o- \mathrm { H } _ { 2 } S abundances relative |
H _ { 2 } |
2.5e-05 |
|
|
1906.09827 🔍 (source)
|
rotates relative |
|
0.1 m as yr-1 |
|
|
1911.02439 🔍 (source)
|
source-lens relative proper motion |
\mu _ { rel } |
9.0 m as yr-1 |
|