FAINT DWARF GALAXIES IN THE NEXT GENERATION VIRGO CLUSTER SURVEY

被引：2
|
作者：
Duc, P-A. [1 ]
Ferrarese, L. [2 ]
Cuillandre, J-C [3 ]
Gwyn, S. [2 ]
MacArthur, L. A. [2 ]
Ferriere, E. [1 ]
Cote, P. [2 ]
Durrell, P. [4 ]
机构：
[1] Univ Paris Diderot, CEA Irfu, CNRS INSU, Lab AIM Paris Saclay, Paris, France
[2] Natl Res Council Canada, Herzberg Inst Astrophys, Ottawa, ON, Canada
[3] Canada France Hawaii Telescope Corp, Kamuela, HI 96743 USA
[4] Youngstown State Univ, Dept Phys & Astron, Youngstown, OH 44555 USA
来源：
CRAL-2010: A UNIVERSE OF DWARF GALAXIES | 2011年 / 48卷
关键词：
LUMINOSITY FUNCTION; POPULATION; EMISSION;
D O I：
10.1051/eas/1148077
中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
The Next Generation Virgo Cluster Survey (NGVS) is a CFHT Large Program that is using the wide field of view capabilities of the MegaCam camera to map the entire Virgo Cluster from its core to virial radius. The observing strategy has been optimized to detect very low surface brightness structures in the cluster, including intracluster stellar streams and faint dwarf spheroidal galaxies. We present here the current status of this ongoing survey, with an emphasis on the detection and analysis of the very low-mass galaxies in the cluster that have been revealed by the NGVS.
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收藏
页码：345 / +
页数：2
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