Paper:	Baryonic Tully-Fisher Relations
Volume:	230, Galaxy Disks and Disk Galaxies
Page:	541
Authors:	McGaugh, S. S.
Abstract:	I describe the disk mass-rotation velocity relation which underpins the familiar luminosity-linewidth relation. Continuity of this relation favors nearly maximal stellar mass-to-light ratios. This contradicts the low mass-to-light ratios implied by the lack of surface brightness dependence in the same relation.

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