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狮子座"原始"环中的巨大恒星形成
David A Thilker1, Jennifer Donovan, David Schiminovich
1Center for Astrophysical Sciences, The Johns Hopkins University, 3400 North Charles Street, Baltimore, Maryland 21218, USA. dthilker@pha.jhu.edu
Nature
|February 20, 2009
概括
狮子座环,一个巨大的气体云,显示了最近恒星形成的迹象,表明它可能是一个形成的矮星系. 这一发现为早期宇宙银河系形成提供了洞察力. 关键词:狮子座环,恒星形成,矮星系,星系形成.
科学领域:
- 天文学和天体物理学
- 宇宙学的宇宙学是什么?
- 银河系的形成和进化
背景情况:
- 星际中性原子 (H i) 云在局部宇宙中很罕见,发现的原始例子很少.
- 狮子座环,一个巨大的结构,是这样一个原始云的候选者,以前只通过辐射观察到.
研究的目的:
- 为了调查狮子座环,寻找恒星群体和正在进行的恒星形成的证据.
- 描述任何检测到的恒星群体的特性,包括金属性和形成时间表.
主要方法:
- 从狮子座环内的气体基结构中检测紫外线.
- 对紫外线可见光度的分析,以限制金属性和恒星形成时间.
主要成果:
- 检测到紫外线,表明最近巨大的恒星形成在狮子座环的气体基层结构.
- 观测到的紫外线颜色表明恒星形成爆发或中度连续恒星形成 (约. 10^8 年).
- 光度学优于低金属度模型 (Z约. Z/50-Z/5),需要进行光谱验证.
结论:
- 狮子座环的基层结构可能代表形成的矮星系缺乏暗物质,类似于潮矮星系,但没有先前的丰富.
- 如果在早期宇宙中很常见,那么这样的结构可能会导致大量未被发现的昏暗,金属贫乏,缺乏光环的矮星系.
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