A Consistent Set of Empirical Scaling Relations for Spiral Galaxies: The - Relations
arXiv:1901.06509 · doi:10.3847/1538-4357/ab1aa4
Abstract
Using the latest sample of 48 spiral galaxies having a directly measured supermassive black hole mass, , we determine how the maximum disk rotational velocity, (and the implied dark matter halo mass, ), correlates with the (i) , (ii) central velocity dispersion, , and (iii) spiral-arm pitch angle, . We find that , significantly steeper than previously reported, and with a root mean square scatter ( dex) similar to that about the - relation for spiral galaxies - in stark disagreement with claims that does not correlate with disks. Moreover, this - relation is consistent with the unification of the Tully-Fisher relation (involving the total stellar mass, ) and the steep relation observed in spiral galaxies. We also find that , consistent with past studies connecting stellar bulges (with ), dark matter halos, and a nonconstant ratio. Finally, we report that , providing a novel formulation between the geometry (i.e., the logarithmic spiral-arm pitch angle) and kinematics of spiral galaxy disks. While the - relation may facilitate distance estimations to face-on spiral galaxies through the Tully-Fisher relation and using as a proxy for , the - relation provides a path for determining dark matter halo masses from imaging data alone. Furthermore, based on a spiral galaxy sample size that is double the size used previously, the self-consistent relations presented here provide dramatically revised constraints for theory and simulations.
25 pages, 3 figures, and 1 table