在NGC 188中,蓝色落后者的质量转移起源由半太阳质量的伴侣揭示出来
Aaron M Geller1, Robert D Mathieu
1Department of Astronomy, University of Wisconsin-Madison, Wisconsin 53706, USA. a-geller@northwestern.edu
Nature
|October 21, 2011
概括
在NGC 188星团中的蓝色落后恒星有伴星,其质量约为太阳的一半. 这一发现支持质量转移作为它们的起源,排除了恒星碰撞.
科学领域:
- 天文学 天文学
- 天体物理学 天体物理学
- 恒星进化 恒星进化
背景情况:
- 蓝色滞留恒星在开放星团中比预期的更亮,更蓝.
- 它们的形成是有争议的,其中包括二进制质量转移,合并和恒星碰撞等假设.
研究的目的:
- 为了研究古老的开放星团NGC 188中蓝色落后恒星的起源.
- 为了区分恒星碰撞和质量转移/聚合场景.
主要方法:
- 在NGC 188星团内的长周期双星中分析蓝色滞后者.
- 确定伴星质量及其分布.
主要成果:
- 在NGC 188中,蓝色落后者拥有伴侣,其质量约为太阳质量的一半.
- 伴侣的狭窄质量分布排除了恒星碰撞的起源.
- 在等级三星的合并只有边际支持.
结论:
- 观察到的伴侣质量强烈支持质量转移作为这些蓝色落后者的主导形成机制.
- 伴侣可能是白矮星,大约有太阳质量的一半.
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