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A FIRST ATTEMPT TO CALIBRATE THE BARYONIC TULLY-FISHER RELATION WITH GAS-DOMINATED GALAXIES
被引:103
作者:
Stark, D. V.
[1
]
McGaugh, S. S.
[2
]
Swaters, R. A.
[2
]
机构:
[1] Univ N Carolina, Dept Phys & Astron, Chapel Hill, NC 27514 USA
[2] Univ Maryland, Dept Astron, College Pk, MD 20742 USA
关键词:
galaxies: dwarf;
galaxies: kinematics and dynamics;
SURFACE BRIGHTNESS GALAXIES;
EXTENDED ROTATION CURVES;
HI IMAGING OBSERVATIONS;
DWARF IRREGULAR GALAXY;
SPIRAL GALAXIES;
MODIFIED DYNAMICS;
STELLAR MASS;
SUPERTHIN GALAXIES;
LOCAL GROUP;
RICH DWARF;
D O I:
10.1088/0004-6256/138/2/392
中图分类号:
P1 [天文学];
学科分类号:
0704 ;
摘要:
We calibrate the baryonic Tully-Fisher (BTF) relation using a sample of gas-dominated galaxies. These determine the absolute scale of the baryonic mass-rotation speed relation independent of the choice of stellar mass estimator. We find a BTF slope of 3.94 +/- 0.07 (random) +/- 0.08 (systematic) and a zero point of 1.79 +/- 0.26 (random) +/- 0.25 (systematic). We apply this relation to estimate the stellar masses of star-dominated galaxies. This procedure reproduces the trend of mass-to-light ratio with color predicted by population synthesis models. The normalization is also correct, consistent with empirical estimates of the initial mass function used in such models.
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页码:392 / 401
页数:10
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