一个观察到的中等质量的恒星群体,已被剥离为二进制恒星
M R Drout1,2, Y Götberg2, B A Ludwig1
1David A. Dunlap Department of Astronomy and Astrophysics, University of Toronto, Toronto M5S 3H4, Canada.
概括
天文学家发现了由二进制相互作用形成的新热星. 这些被剥离的恒星可能是被剥离的超新星的祖先,填补了恒星进化知识的空白.
科学领域:
- 恒星天体物理学
- 双星演变
背景情况:
- 巨大的恒星可以通过二进制相互作用失去包裹.
- 理论模型预测来自这个过程的热恒星 (2-8个太阳质量).
- 在此之前, 只有一个这样的星系被确定.
研究的目的:
- 为了识别和描述潜在的星.
- 通过二进制脱落模型预测恒星的属性.
- 了解二进制星系中大质量恒星的演化过程.
主要方法:
- 使用紫外线光度测量来识别被剥离的恒星.
- 在25个候选恒星上进行光学光谱.
- 分析了恒星属性,包括温度,表面重力和表面组成.
主要成果:
- 确定了16颗表现出二进制运动的恒星.
- 证实了高温 (~60,000-100,000 K) 和高表面重力.
- 观察到缺少的表面, 符合剥离的包裹.
- 发现这些恒星的初始质量为8-25太阳质量, 弥合了已知的恒星类型之间的差距.
结论:
- 这些已识别的恒星与二进制星的理论预测一致.
- 这些恒星代表了小矮恒星和狼雷耶恒星之间的恒星进化中缺失的环节.
- 发现的群体被认为是剥离外超新星的祖先.
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