Spatial distribution of spiral galaxies in the Virgo Cluster from the Tully-Fisher relation

1993 ◽  
Vol 412 ◽  
pp. L13 ◽  
Author(s):  
M. Fukugita ◽  
S. Okamura ◽  
N. Yasuda
Keyword(s):  
Spatial Distribution ◽  
Spiral Galaxies ◽  
Virgo Cluster ◽  
Fisher Relation

The mass-to-light ratios of low surface brightness spiral galaxies: Clues from the Tully-Fisher relation

1995 ◽  
Vol 438 ◽  
pp. 72 ◽  
Author(s):  
D. Sprayberry ◽  
G. M. Bernstein ◽  
C. D. Impey ◽  
G. D. Bothun
Keyword(s):  
Surface Brightness ◽  
Spiral Galaxies ◽  
Low Surface Brightness ◽  
Fisher Relation

scholarly journals THE STELLAR POPULATIONS OF STRIPPED SPIRAL GALAXIES IN THE VIRGO CLUSTER

2008 ◽  
Vol 136 (4) ◽  
pp. 1623-1644 ◽  
Author(s):  
Hugh H. Crowl ◽  
Jeffrey D. P. Kenney
Keyword(s):  
Spiral Galaxies ◽  
Stellar Populations ◽  
Virgo Cluster

scholarly journals The Tully-Fisher relation: evolution with redshift and environment

2006 ◽  
Vol 2 (S235) ◽  
pp. 8-11 ◽  
Author(s):  
Alfonso Aragón-Salamanca
Keyword(s):  
Spiral Galaxies ◽  
Rotation Velocity ◽  
Disk Galaxies ◽  
Cluster Galaxies ◽  
Fundamental Properties ◽  
Look Back ◽  
Formation And Evolution ◽  
Fisher Relation

AbstractThe Tully-Fisher Relation (TFR) links two fundamental properties of disk galaxies: their luminosity and their rotation velocity (mass). The pioneering work of Vogt et al. in the 1990's showed that it is possible to study the TFR for spiral galaxies at considerable look-back-times, and use it as a powerful probe of their evolution. In recent years, several groups have studied the TFR for galaxies in different environments reaching redshifts beyond one. In this brief review I summarise the main results of some of these studies and their consequences for our understanding of the formation and evolution of disk galaxies. Particular emphasis is placed on the possible environment-driven differences in the behaviour of the TFR for field and cluster galaxies.

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