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.
引用
收藏
页码:392 / 401
页数:10
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