Interpreting Offsets from the Tully-Fisher Relation

Details Interpreting Offsets from the Tully-Fisher Relation Interpreting Offsets from the Tully-Fisher Relation

2002-06-05

arxiv.org/abs/astro-ph/0206088v1

Rev.Mex.Astron.Astrof.Ser.Conf.17:188,2003

Astronomy and Astrophysics

Astrophysics

1 page including 2 figures, to appear in proceedings of "Galaxy Evolution: Theory and Observations," eds. Avila-Reese, Firmani

Scientific paper

We have previously demonstrated that Tully-Fisher residuals correlate with
tracers of star formation history (color and emission line equivalent width)
for a broad sample of Sa--Sd spiral galaxies (Kannappan, Fabricant, & Franx
2002). Here we use these correlations to study two other classes of galaxies:
(1) galaxies in close pairs and (2) galaxies at intermediate redshift.

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