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有证据表明,Ia型超新星有两个不同的群体
Xiaofeng Wang1, Lifan Wang, Alexei V Filippenko
1Department of Physics, Tsinghua University, Beijing, China. wang_xf@mail.tsinghua.edu.cn
概括
类型Ia超新星的起源仍然是未知的. 这项研究将超新星的光谱多样性与它们的主星系环境联系起来,这表明高速超新星的年轻,富含金属的祖先.
科学领域:
- 测量宇宙膨胀的方法
- 恒星进化中的恒星演变
- 银河系环境 银河系环境
背景情况:
- 一类超新星 (SNe Ia) 是宇宙学的关键标准.
- 人们还不太了解SNe Ia的祖先.
- 了解SN Ia的起源是完善宇宙膨胀测量的关键.
研究的目的:
- 研究SN Ia光谱多样性与它们的出生环境之间的关系.
- 确定祖先属性是否与宿主星系特征相关.
- 提供有关不同类型SNIA的起源的见解.
主要方法:
- 分析了SNe Ia的光谱多样性.
- 相关的超新星属性 (例如,射出速度) 与宿主星系属性 (例如,区域,亮度,大小).
- 根据环境相关性推导的原始特征.
主要成果:
- 高速度的SNeIa集中在内部,更明亮的星系区域.
- 高速度的SNe Ia是在更大,更亮的宿主星系中发现的.
- 在SNe Ia的光谱多样性与出生地环境有关.
结论:
- 高速度的SNe Ia很可能来自更年轻,更富含金属的祖先.
- SNe Ia 的原始群体受宿主星系属性的影响.
- 银河系的化学进化在SN Ia的祖先形成中发挥了作用.
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