长玛射线爆发后的一颗富含兰他尼德的千诺瓦
Yu-Han Yang1, Eleonora Troja2,3, Brendan O'Connor4,5,6
1Department of Physics, University of Rome "Tor Vergata", Rome, Italy. yuhan.yang@roma2.infn.it.
Nature
|February 21, 2024
概括
基隆新星,来自合并物体的宇宙爆炸, 显示晚期行为由冷却的化物丰富的喷射物解释. 这项研究分析了马射线爆发230307A
科学领域:
- 天体物理学
- 多波长天文学
背景情况:
- 千新星是短暂的天体物理事件,由重元素在紧的物体合并中合成的放射性衰变提供动力.
- 它们的晚期行为 (数周到数月) 取决于排泄物组成和合并残留物.
- 与射爆发230307A相关的千新星与AT2017gfo有相似之处,中红外光谱表明存在.
研究的目的:
- 进行与玛射线爆发230307A相关的千诺瓦多波长分析.
- 模拟千新星在爆炸后的两个月的演变.
- 调查控制晚期千诺瓦排放的物理过程.
主要方法:
- 使用公开的詹姆斯·韦伯太空望远镜数据.
- 纳入哈勃太空望远镜的观测数据.
- 模拟了千新星的演变,包括光球半径衰退和玻利米度亮度衰减.
主要成果:
- 千诺瓦的光球半径随着时间的推移而衰退.
- 观察到玻利米度亮度的快速衰减 (Lbol t-2.7±0.4).
- 这些晚期观测支持冷却,富含兰他化物排泄物的重组.
结论:
- 来自马射线爆发230307A的基隆新星的晚期演变与富含胺物质的冷却和重组相一致.
- 这提供了重元素合成在千新星事件中的作用的进一步证据.
- 多波长的观测对于在不同的时间尺度上理解千新星物理学至关重要.
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