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在处女座星团中检测出一个集群内部球状星团的大规模结构
Myung Gyoon Lee1, Hong Soo Park, Ho Seong Hwang
1Astronomy Program, Department of Physics and Astronomy, Seoul National University, Seoul 151-742, Korea. mglee@astro.snu.ac.kr
星团内部球状星团 (IGC) 在处女座星团中发现,延伸数百万光年. 这些结构比星系更大,很可能起源于被剥离的矮星系.
科学领域:
- 天文学和天体物理学
- 银河系的进化 银河系的进化
- 暗物质研究 暗物质研究
背景情况:
- 球状星团通常位于星系内.
- 集群内部球状星团 (IGCs) 被假设存在,与星系集群相结合,而不是单个星系.
- 球状星团是绘制暗物质分布的关键标志物.
研究的目的:
- 调查处女座星团内集群内部球状星团 (IGC) 的存在和分布.
- 在整个处女座星团中绘制球状星团的大规模分布图.
- 了解政府间会议的起源和形成机制.
主要方法:
- 在处女座星团内绘制球状星团的空间分布.
- 分析已识别的IGC子结构的规模和度.
- 将IGC分布与星系结构和理论模型进行比较.
主要成果:
- 在处女座星团星团中生成了球状星团分布的全面地图.
- 检测到的IGC从处女座星团中心延伸至500万光年.
- 在比单个星系大得多的子结构中观察到显著的IGC度.
结论:
- 这项研究证实了处女座星团中存在集群内部球状星团 (IGCs).
- 这些IGC分布在巨大的尺度上,表明超出单个星系之外的显著人口.
- 这些发现表明,IGC可能主要来自被剥夺了恒星内容的矮星系.
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