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Published on: November 15, 2013
在一个巨大的恒星星团中排除了相当大的年龄范围
Chengyuan Li1, Richard de Grijs2, Licai Deng3
11] Kavli Institute for Astronomy and Astrophysics, Peking University, Yi He Yuan Lu 5, Hai Dian District, Beijing 100871, China [2] Department of Astronomy, Peking University, Yi He Yuan Lu 5, Hai Dian District, Beijing 100871, China [3] Key Laboratory for Optical Astronomy, National Astronomical Observatories, Chinese Academy of Sciences, 20A Datun Road, Chaoyang District, Beijing 100012, China.
大质量恒星星团中的扩展主序关闭区域可能不表明年龄差异. 快速旋转的恒星为这些特征提供了合理的解释,挑战了以前对恒星群体的解释.
科学领域:
- 天文学和天体物理学.
- 恒星进化中的恒星演变
- 恒星星团动态 恒星团动态
背景情况:
- 巨大的中年恒星星团经常表现出扩展的主序关闭 (eMSTO) 区域.
- eMSTO通常被解释为具有显著内部年龄差距 (数亿年) 的证据.
- 据认为,年轻星团会迅速排出恒星形成燃料,从而限制年龄分散.
研究的目的:
- 为了调查中年星团中eMSTOs的原因.
- 确定eMSTO是否必然意味着内部年龄分散.
- 探索eMSTO形态学的替代解释.
主要方法:
- 恒星星团NGC 1651的高分辨率成像观测.
- 恒星群的理论建模. 恒星群的理论建模.
- 对多个星团的赫茨普朗格-拉塞尔图的分析.
主要成果:
- 在20亿年前的星团NGC 1651 (1.7 × 10^5太阳质量) 中的eMSTO与单个年龄的恒星群体一致.
- 快速旋转的恒星被认为是观测到eMSTO的最合理的解释.
- 在至少五个其他中年星团中观察到类似的eMSTO形态.
结论:
- 扩展的主序关闭区域并不一定表明恒星团的内部年龄分散是显著的.
- 快速旋转的恒星可能是导致eMSTOs的常见现象.
- 需要进一步的研究才能充分理解快速旋转的恒星对恒星生命周期和星团演变的影响.
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