在年轻的超新星残留物Cassiopeia A中发现
Bon-Chul Koo1, Yong-Hyun Lee, Dae-Sik Moon
1Department of Physics and Astronomy, Seoul National University, Seoul 151-747, Korea.
概括
超新星 (SNe) 产生,是生命至关重要的元素. 对卡西欧佩亚A的观测显示,与铁的比率高达银河系平均值的100倍,这证实了SN的产生.
科学领域:
- 天文学 天文学
- 天体物理学 天体物理学
- 核天体物理学 核天体物理学
背景情况:
- (P) 对于生命至关重要,并被认为是在大质量恒星中合成的.
- 超新星 (SNe) 假设将合成的分散到星际空间.
研究的目的:
- 通过分析其在超新星残骸中的丰富度来调查的起源.
- 确认超新星在核合成中的作用.
主要方法:
- 近红外光谱观测Cassiopeia A超新星残余的近红外光谱观测.
- 在SN材料中对 (P) 与铁 (Fe) 的丰度比率分析.
主要成果:
- 卡西欧佩亚A射出的与铁的比率高达银河系平均水平的100倍.
- 这一发现证实了超新星会产生.
- 观察到的比率与核合成模型一致,但与完整的混合场景相矛盾.
结论:
- 作为超新星爆炸的大型恒星被证实是的重要来源.
- 观测到的丰度比率为超新星爆炸和混合动力学提供了限制.
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