VLA Observations and Tully-Fisher Distances of Gas-poor Spiral Galaxies in the Virgo Cluster Region

2008 ◽  
Author(s):  
M. C. Toribio ◽  
Robert Minchin ◽  
Emmanuel Momjian
Keyword(s):  
Spiral Galaxies ◽  
Virgo Cluster ◽  
Cluster Region

Surface photometry of spiral galaxies in the Virgo cluster region

1995 ◽  
Vol 96 ◽  
pp. 359 ◽  
Author(s):  
Naoki Yasuda ◽  
Sandanori Okamura ◽  
Masataka Fukugita
Keyword(s):  
Spiral Galaxies ◽  
Virgo Cluster ◽  
Surface Photometry ◽  
Cluster Region

scholarly journals Results From VLA Observations of Five Spiral Galaxies In The Virgo Cluster Region

2006 ◽  
Vol 2 (S235) ◽  
pp. 245-245
Author(s):  
M. C. Toribio ◽  
J. M. Solanes
Keyword(s):  
Spiral Galaxies ◽  
Virgo Cluster ◽  
High Density ◽  
Large Array ◽  
Interstellar Gas ◽  
Ongoing Debate ◽  
Very Large Array ◽  
Cluster Region ◽  
Neutral Gas ◽  
Cluster Environment

AbstractNew HI synthesis observations have been made for the five spiral galaxies NGC 4307, NGC 4356, NGC 4411a/b and NGC 4492, located in the Virgo Cluster Region, with the Very Large Array in its CS configuration. All these objects, but NGC 4411a, belong to a sample of spirals identified in previous single-dish studies of the HI distribution within the Virgo Cluster and its outskirts. The thirteen members of that sample were selected for showing neutral gas deficiencies as strong as those of the inner galaxies of Virgo and other rich clusters, but apparently lying on the infall region.The goal of the present observations is to progress further on the identification of the external mechanisms that may be responsible for the reduction of the interstellar gas in spiral galaxies and thus contribute to the study of the evolution of galaxies in high-density environments. In particular, the results of this work are relevant for the ongoing debate on the pre-processing of galaxies prior to entering the cluster environment.

scholarly journals Optical Search of Faint IRAS Point Sources in the Virgo Cluster Region

1990 ◽  
Vol 139 ◽  
pp. 373-374
Author(s):  
X. T. He ◽  
K. Liang ◽  
K. Huang
Keyword(s):  
Intergalactic Medium ◽  
Infrared Emission ◽  
Virgo Cluster ◽  
Point Sources ◽  
Cluster Region ◽  
Extensive Region ◽  
Strongly Connected

The infrared emission in galaxies is strongly connected to star burst processes, while emission from the intergalactic medium results mainly from dust heated by other luminosity sources. The Virgo cluster provides an extensive region in which the properties of such infrared emission can be studied. Galaxies in the Virgo cluster with dust temperatures of 40 K and masses of dust as small as about 5 × 104M⊙ are detectable at the limit of the IRAS survey (Soifer et al., 1987). The IRAS observations of 196 optically selected galaxies in the Virgo cluster have been studied by Helou et al. (Helou et al., 1988; see also Leggett et al., 1988).

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
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