在IRC+10216周围发现了水蒸气,作为彗星绕另一个恒星运行的证据
G J Melnick1, D A Neufeld, K E Saavik Ford
1Harvard-Smithsonian Center for Astrophysics, 60 Garden Street, Cambridge, Massachusetts 02138, USA. gmelnick@cfa.harvard.edu
Nature
|July 13, 2001
概括
天文学家在碳星IRC+10216周围探测到水蒸气,这是一个意想不到的发现. 这表明,由于恒星最近的亮度增加,轨道上的冰体正在蒸发.
科学领域:
- 天文学和天体物理学
- 外系行星科学 外系行星科学
背景情况:
- 自1995年以来,木星质量系外行星已经通过恒星反射运动被检测出来,这是从光谱变化中推断出来的.
- 这种辐射速度方法不足以检测较小的太阳系类型的天体.
研究的目的:
- 为了研究进化碳星IRC+10216.6周围环恒星物质的组成.
- 探索探测较小轨道天体的替代方法.
主要方法:
- 使用光谱分析观测环恒星水蒸气.
- 分析已进化的碳星IRC+10216的亮度变化.
主要成果:
- 在IRC+10216.6的环恒星环境中检测出显著的水蒸气.
- 在碳星周围,水蒸气通常不会在可测量的数量中出现.
结论:
- 观测到的水蒸气强烈地暗示了轨道上的冰体的蒸发.
- 这种现象与最近IRC+10216的亮度显著增加有关.
- 这些发现支持冰体蒸发在演化中的恒星周围的理论模型.
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