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来自对25亿年前星团观测的冷恒星的回转向下的时钟
Søren Meibom1, Sydney A Barnes2, Imants Platais3
1Harvard-Smithsonian Center for Astrophysics, Cambridge, Massachusetts 02138, USA.
Nature
|December 25, 2014
概括
确定恒星年龄是一项挑战. 这项研究使用NGC 6819中冷恒星的旋转速率校准了陀螺计时,使得许多恒星能够精确地确定年龄.
科学领域:
- 天文学和天体物理学
- 恒星进化 恒星进化
- 银河系的动力学
背景情况:
- 恒星年龄对于理解恒星进化和银河系历史至关重要.
- 传统的恒星约会方法对于低质量 (冷) 恒星通常是不可靠的,因为属性变化缓慢或测量难度很大.
- 基于恒星旋转速率的陀螺年代学,为年龄确定提供了一个有前途的替代方案.
研究的目的:
- 通过建立旋转周期,恒星质量和年龄之间的关系来校准低质量恒星的陀螺计时方法.
- 为了测试回旋计时学对较老恒星群体的可靠性.
主要方法:
- 测量了25亿年前的开放星团NGC 6819.9中的30颗冷恒星的旋转周期.
- 分析测量的旋转周期和星团内的恒星质量之间的关系.
主要成果:
- 对于星团年龄的冷恒星,确定了旋转周期和恒星质量之间的明确关系.
- 这种校准可使年龄的确定精确度达到约10%.
结论:
- 陀螺计时是确定冷恒星年龄的可靠方法,即使在老年群体中也是如此.
- 这些发现允许对众多银河系场恒星进行精确的年龄评估,推进恒星和银河系研究.
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