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在银河系的核膨胀中,有三颗古典的 Cepheid 变星
Noriyuki Matsunaga1, Takahiro Kawadu, Shogo Nishiyama
1Kiso Observatory, Institute of Astronomy, University of Tokyo, 10762-30 Mitake, Kiso-machi, Kiso-gun, Nagano 397-0101, Japan. matsunaga@ioa.s.u-tokyo.ac.jp
Nature
|August 26, 2011
概括
在银河系的核膨胀中恒星形成是偶尔发生的. 最近爆发的恒星形成,以古典的Cepheid变量表示,表明活动大约2500万年前.
科学领域:
- 天文学 天文学
- 天体物理学 天体物理学
- 银河系进化 银河系进化
背景情况:
- 银河系的核膨胀,一个半径约200帕塞克的中心区域,有一个复杂的恒星形成历史.
- 了解这个地区恒星形成的触发因素和时间对于银河系进化模型至关重要.
- 经典的塞菲德变量提供了一种方法,可以根据它们的周期-年龄关系来确定恒星形成的日期.
研究的目的:
- 为了调查银河系核膨胀的近期恒星形成历史.
- 为了确定在银河系中心附近增加恒星形成活动的特定时期.
主要方法:
- 利用经典的Cepheid变星作为探测恒星形成历史的探测器.
- 分析了中央黑洞40帕塞克内发现的塞菲德星脉动周期的分布.
主要成果:
- 在核膨胀中检测到三颗经典的星座,其脉冲周期大约为20天.
- 在这个特定区域没有观察到有明显较长或较短周期的星座.
- 推断了大约2500万年前增加恒星形成的时期,可能延伸到最近.
结论:
- 核膨胀经历了偶尔的恒星形成,大约2500万年前出现了显著的爆发.
- 这次最近的爆发与3千万到7千万年前的较不活跃时期形成鲜明对比.
- 这些发现支持了由银河系中心气体含量波动驱动的周期性恒星形成模型.
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