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一个极其冷的白矮星的红外光谱
1Department of Physics and Astronomy, University of Leicester, UK. sth@ast.cam.ac.uk
Nature
|January 19, 2000
概括
天文学家发现已知最冷的白矮星,这颗恒星经过数十亿年的冷却. 这一发现支持了这些恒星残骸可能构成银河系的理论.
科学领域:
- 天文学和天体物理学
- 恒星进化 恒星进化
- 宇宙学的宇宙学是什么?
背景情况:
- 白矮星是从初始质量低于8太阳质量的恒星中形成的末期恒星残留物.
- 这些物体经过数十亿年的冷却,理论上构成了银河系暗物质光环的很大一部分.
- 检测极度冷的白矮星是具有挑战性的,因为它们的淡度和光谱与其他矮星相似.
研究的目的:
- 为了研究极其寒冷的白矮星的性质和特性.
- 为了测试最近的理论模型,预测这些恒星的蓝色.
- 评估白矮星对银河系暗物质的贡献.
主要方法:
- 获取和分析一个极其冷的白矮星的红外光谱.
- 使用光谱数据确定恒星的温度.
- 动力学分析以确定恒星在银河系内的位置.
主要成果:
- 红外光谱与预测蓝色白矮星的新模型一致.
- 恒星的温度被确定为3,500 +/- 200 K,确定它是已知的最冷的白矮星.
- 这颗恒星的动力学将其置于银河系的光环中.
结论:
- 这颗凉爽的白矮星的发现验证了最新的恒星模型.
- 这些物体的推断密度支持了白矮星主导银河系光环暗物质的假设.
- 这一发现对了解银河系的组成和暗物质分布有重大影响.
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