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从大麦哲伦云中的古代超新星中发出的光回声
Armin Rest1, Nicholas B Suntzeff, Knut Olsen
1Cerro Tololo Inter-American Observatory, National Optical Astronomy Observatory, La Serena, Chile.
Nature
|December 24, 2005
概括
科学家在大麦哲伦云中检测到历史上的超新星的光回声. 这些回声有助于确定超新星的年龄和类型,为宇宙爆炸提供了新的见解.
科学领域:
- 天文学和天体物理学
- 太空爆炸 太空爆炸
- 超新星残留物 超新星残留物
背景情况:
- 超新星光回声,即过去爆炸的散射光,可以揭示超新星的位置,年龄和类型.
- 虽然已知存在银河系外的回声,但对于历史上的银河系超新星,没有发现过任何回声.
- 在银河系中寻找超新星光回声的搜索一直没有成功.
研究的目的:
- 为了寻找和识别超新星,在大麦哲伦星云中寻找和识别历史超新星的光回声.
- 用回声特性确定这些历史超新星的年龄和类型.
主要方法:
- 在大麦哲伦云中观测微弱的,可变的表面亮度复合体.
- 对这些复合体的看似自动运动进行分析.
- 利用距离和正确运动数据来估计回声年龄.
主要成果:
- 发现了三种与小,可能是年轻超新星残骸相关的光回声候选者.
- 这些残骸被认为是Ia型超新星.
- 对于两个已识别的回声,估计年龄为610年和410年.
结论:
- 这些光回声的检测提供了大麦哲伦云中历史上的超新星的证据.
- 这种方法允许在初始事件发生后很长时间研究超新星特征.
- 它为研究我们银河系附近超新星的历史开辟了新的途径.
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