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19952001
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astro-ph2001

High-resolution rotation curves of LSB galaxies: Mass Models

Erwin de Blok, Stacy McGaugh, Vera Rubin

We present mass models for a sample of 30 high-resolution rotation curves of low surface brightness (LSB) galaxies. We fit both pseudo-isothermal (core-dominated) and Cold Dark Mat…

astro-ph2000

Baryonic Tully-Fisher Relations

Stacy McGaugh

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-li…

astro-ph1999

Dynamical Constraints on Disk Galaxy Formation

Stacy McGaugh

The rotation curves of disk galaxies exhibit a number of striking regularities. The amplitude of the rotation is correlated with luminosity (Tully-Fisher), the shape of the rotatio…

astro-ph1998

How Galaxies Don't Form

Stacy McGaugh

I review current theories of disk galaxy formation. All fail in the light of recent data for low surface brightness galaxies. The difficulty stems from the presence of a unique acc…

astro-ph1998

Optical Galaxy Selection

Stacy McGaugh

Our view of the properties of galaxies is strongly affected by the way in which we survey for them. I discuss some aspects of selection effects and methods to compensate for them.…

astro-ph1997

The Baryon Fraction Distribution and the Tully-Fisher Relation

Stacy McGaugh, Erwin de Blok

A number of observations strongly suggest that the baryon fraction is not a universal constant. One obvious interpretation is that there is some distribution of Fb, and the differe…