Homogeneous Photometry for Star Clusters and Resolved Galaxies. I. A Survey of Bright Stars in the Fornax Dwarf Spheroidal Galaxy

Homogeneous Photometry for Star Clusters and Resolved Galaxies. I. A Survey of Bright Stars in the Fornax Dwarf Spheroidal Galaxy
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星团和分辨星系的均匀光度测量。

DOI:
10.1086/316164
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发表时间:
1998
影响因子:
3.5
通讯作者:
T. Smecker
T. Smecker
中科院分区:
物理与天体物理3区
文献类型:
--
作者:
P. Stetson;J. Hesser;T. Smecker

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我们在约翰逊B,Kron-Einins R测光系统上为大约100,000颗恒星提供了精确的测光,这些恒星位于天炉座矮球状星系中心的1 / 3 deg 2区域。我们发现了许多可能的短周期变星,蓝色恒星似乎是一个小群体的主要序列,年龄约为108年,和两种不同类型的发光红色星星:一个主要是碳星的扩展序列和一群主要是M巨星,比巨型分支尖端稍微更明亮。被认为是在天炉座矮星系的空间分布,这些子群。
We present accurate photometry on the Johnson B, Kron‐Cousins R photometric system for approximately 100,000 stars in a 1 / 3 deg2 field centered on the dwarf spheroidal galaxy in Fornax. We identify numerous probable short‐period variable stars, blue stars that appear to be the main sequence of a small population with an age of order 108 yr, and two distinct types of luminous red star: an extended sequence of primarily carbon stars and a clump of mostly M giants slightly more luminous than the giant‐branch tip. The spatial distribution of each of these subpopulations within the Fornax dwarf galaxy is considered.