LEO V: A COMPANION OF A COMPANION OF THE MILKY WAY GALAXY?

被引:133
作者
Belokurov, V. [1 ]
Walker, M. G. [1 ]
Evans, N. W. [1 ]
Faria, D. C. [1 ]
Gilmore, G. [1 ]
Irwin, M. J. [1 ]
Koposov, S. [2 ]
Mateo, M. [3 ]
Olszewski, E. [4 ]
Zucker, D. B. [1 ]
机构
[1] Univ Cambridge, Inst Astron, Cambridge CB3 0HA, England
[2] Max Planck Inst Astron, D-69117 Heidelberg, Germany
[3] Univ Michigan, Dept Astron, Ann Arbor, MI 48109 USA
[4] Univ Arizona, Steward Observ, Tucson, AZ 85721 USA
基金
美国国家科学基金会; 美国国家航空航天局; 英国科学技术设施理事会;
关键词
galaxies: dwarf; galaxies: individual (Leo); Local Group;
D O I
10.1086/592962
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We report the discovery of a new Milky Way satellite in the constellation Leo, identified in data from the Sloan Digital Sky Survey. It lies at a distance of similar to 180 kpc, and is separated by less than or similar to 3 degrees from another recent discovery, Leo IV. We present follow-up imaging from the Isaac Newton Telescope and spectroscopy from the Hectochelle fiber spectrograph at the Multiple Mirror Telescope. Leo V's heliocentric velocity is similar to 173.3 +/- 3.1 km s(-1), offset by similar to 40 km s(-1) from that of Leo IV. A simple interpretation of the kinematic data is that both objects may lie on the same stream, although the implied orbit is only modestly eccentric (e similar to 0.2)
引用
收藏
页码:L83 / L86
页数:4
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