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来自银河系中大质量恒星的放射性26Al
Roland Diehl1, Hubert Halloin, Karsten Kretschmer
1Max-Planck-Institut für extraterrestrische Physik, D-85748 Garching, Germany. rod@mpe.mpg.de
Nature
|January 7, 2006
概括
放射性-26 (26Al) 马射线显示正在进行的宇宙核合成. 测量证实26Al起源于整个银河系,支持每世纪大约2个超新星的速度.
科学领域:
- 天体物理学 天体物理学
- 核天体物理学 核天体物理学
- 宇宙射线物理学 宇宙射线物理学
背景情况:
- 放射性26Al (半衰期~7.2 x 10^5年) 玛射线为银河系核合成提供了洞察力.
- 之前的研究表明,26Al的起源是整个银河系和本地起源,基于玛射线辐射和石数据.
研究的目的:
- 为了研究26Al在银河系的起源和分布.
- 为了确定银河系核合成速率和核心崩超新星的频率.
主要方法:
- 在1808.65 keV的26Al马射线辐射的高光谱分辨率测量.
- 对玛射线发射模式的分析,以推断源区域动态.
主要成果:
- 发现26Al的发射区域与银河系相结合,支持整个银河系的起源.
- 确定26Al的当前平衡质量为2.8 (+/- 0.8) 太阳质量.
- 核心崩超新星的频率估计为每世纪1.9 (+/- 1.1) 事件.
结论:
- 整个银河系的大型恒星是26Al的主要生产者.
- 观测到的26Al分布和动态支持一个全银河系核合成模型.
- 估计的超新星速率为银河系化学进化模型提供了关键数据.
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