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The K-band Tully-Fisher Relation for Compact Groups

Author(s):
Torres-Flores, S. ; Mendes de Oliveira, C. ; Amram, P. ; Plana, H. ; VerdesMontenegro, L ; DelOlmo, A ; Sulentic, J
Total Authors: 7
Document type: Journal article
Source: GALAXIES IN ISOLATION: EXPLORING NATURE VERSUS NURTURE; v. 421, p. 1-pg., 2010-01-01.
Abstract

We present results on the Tully-Fisher relation of galaxies in dense environments as compared to galaxies in the field. Our main result is that galaxies in Hickson compact groups (HCG) lie on the K-band Tully-Fisher relation defined by galaxies in less dense environments (GHASP survey) although with more scatter. However, some of the lowest mass systems (e.g. 49b) have a mass that is too low for their stellar luminosities. These galaxies could have their dark halos truncated due to interactions. (AU)

FAPESP's process: 07/07973-3 - The internal kinematics of galaxies in Hickson compact groups
Grantee:Sergio Patricio Torres Flores
Support Opportunities: Scholarships in Brazil - Doctorate (Direct)