Tidal Remnants Around the Galactic Globular Clusters NGC 1851 and NGC 1904

被引：7
|
作者：
Carballo-Bello, J. A. [1 ]
Martinez-Delgado, D. [1 ]
机构：
[1] Inst Astrofis Canarias, San Cristobal la Laguna 38205, Spain
来源：
HIGHLIGHTS OF SPANISH ASTROPHYSICS V | 2010年
关键词：
D O I：
10.1007/978-3-642-11250-8_90
中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
Deep photometry around the Galactic globular clusters NGC 1851 and NGC 1904 obtained with the Wide Field Imager in the 2.2 m ESO telescope reveals a distinct main-sequence of a metal-poor stellar population, consistent with the presence of a very low surface brightness stellar system. The unveiled population might belong to an unknown tidal stream in the Milky Way but other possibilities are here discussed.
引用
收藏
页码：383 / 383
页数：1
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