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来自大麦哲伦星云中的一个巨大的年轻恒星的帕塞克尺度光学喷射
Anna F McLeod1, Megan Reiter2, Rolf Kuiper3
1School of Physical and Chemical Sciences, University of Canterbury, Christchurch, New Zealand.
Nature
|January 25, 2018
概括
天文学家发现HH 1177,来自大马格伦星云中的一个巨大的年轻恒星的光学喷射. 这一发现表明喷气发射和聚合的物理是普遍的, 无论恒星质量如何.
科学领域:
- 天体物理学
- 恒星进化
- 恒星形成
背景情况:
- 年轻的恒星物体 (YSOs) 经常表现出高度聚合的喷气,通常与积累盘相关.
- 在高质量恒星中,磁盘介导的积累越来越多,尽管它们的形成仍然不清楚.
- 在此之前,大质量恒星的喷射在光学波长或银河系之外没有被观测到,这是由于遮蔽.
研究的目的:
- 在银河系外的一颗巨大的年轻恒星物体中发现了光学电离喷气.
- 为了研究这颗喷射对大质量恒星形成理论的特性和影响.
- 测试喷气发射和聚合物理是独立于恒星质量的假设.
主要方法:
- 对HH 1177喷气式飞机的光学观察.
- 分析喷气流的结合,几何和起源.
- 与已知来自低质量年轻恒星物体的喷气相比较.
主要成果:
- 发现HH 1177,一个高度聚合的双极光学离子喷气.
- 喷射源于一个巨大的年轻恒星物体在大麦哲伦云.
- 喷气至少延伸到十个帕塞克, 表明正在进行的盘介导积累.
结论:
- 观测到的喷气提供了大质量恒星中盘介积的证据.
- 星系的形成很可能跟随了小质量的恒星形成机制的扩大版本.
- 控制喷气发射和聚合的物理似乎与恒星质量无关.
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