Interpreting Offsets from the Tully-Fisher Relation

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dc.creatorKannappan, S. J.
dc.creatorGillespie, E. Barton
dc.creatorFabricant, D. G.
dc.creatorFranx, M.
dc.creatorVogt, N. P.
dc.date2002-06-05
dc.date.accessioned2026-07-07T10:31:16Z
dc.date.available2026-07-07T10:31:16Z
dc.descriptionWe 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.
dc.description1 page including 2 figures, to appear in proceedings of "Galaxy Evolution: Theory and Observations," eds. Avila-Reese, Firmani, Frenk, and Allen; RevMexAA SC style files included
dc.identifierhttps://arxiv.org/abs/astro-ph/0206088
dc.identifierhttp://arxiv.org/abs/astro-ph/0206088
dc.identifierRev.Mex.Astron.Astrof.Ser.Conf.17:188,2003
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/178354
dc.subjectAstrophysics
dc.titleInterpreting Offsets from the Tully-Fisher Relation
dc.typetext

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