行星星云Henize 2-428的双重退化,超级Chandrasekhar核心的行星星云
M Santander-García1, P Rodríguez-Gil2, R L M Corradi2
11] Observatorio Astronómico Nacional, Apartado de Correos 112, E-28803, Alcalá de Henares, Spain [2] Instituto de Ciencia de Materiales de Madrid (CSIC), Sor Juana Inés de la Cruz, 3, E-28049 Madrid, Spain.
Nature
|February 18, 2015
概括
天文学家发现了一个双退化恒星系统,Henize 2-428,其质量超过了Chandrasekhar极限. 这一发现支持超级Chandrasekhar型Ia超新星的双重退化途径.
科学领域:
- 天体物理学 天体物理学
- 恒星进化 恒星进化
- 星球星云是行星星云.
背景情况:
- 行星星云由1-8M的恒星形成.
- 复杂的行星星云形态不太清楚,二进制相互作用作为一种拟议的机制.
- 双退化系统由两个白矮星组成,它们已经抛出了它们的包裹.
研究的目的:
- 研究复杂的行星星云形态的起源.
- 确定类型Ia超新星的进化途径.
- 分析Henize 2-428系统的情况.
主要方法:
- 观测天文学是一种观测天文学.
- 恒星进化模型的建模
- 分析二进制系统参数 (质量,轨道周期).
主要成果:
- 赫尼泽2-428是一个双退化系统,总质量约为1.76M.
- 这种质量超过了Chandrasekhar的1.4M的极限.
- 该系统的轨道周期短4.2小时,预计将在7亿年内合并.
结论:
- 赫尼兹2-428系统支持Ia型超新星的双重退化,超级钱德拉塞哈尔进化途径.
- 这一发现为超新星形成的关键机制提供了观测证据.
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