Baryonic Tully-Fisher Relations

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dc.creatorMcGaugh, Stacy
dc.date2000-09-20
dc.date.accessioned2026-07-07T01:55:33Z
dc.date.available2026-07-07T01:55:33Z
dc.descriptionI 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.
dc.description4 pages including 1 figure. Invited review for "Galaxy Disks and Disk Galaxies", eds. J.G. Funes S.J. & E.M. Corsini
dc.identifierhttps://arxiv.org/abs/astro-ph/0009338
dc.identifierhttp://arxiv.org/abs/astro-ph/0009338
dc.identifierASP Conf.Ser. 230 (2001) 541-544
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/1695
dc.subjectAstrophysics
dc.titleBaryonic Tully-Fisher Relations
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