通过无线电检测到含有丰富的环恒星物质的Ia型超新星
Erik C Kool1, Joel Johansson2,3, Jesper Sollerman2
1The Oskar Klein Centre, Department of Astronomy, Stockholm University, AlbaNova, Stockholm, Sweden. erik.kool@astro.su.se.
Nature
|May 17, 2023
概括
天文学家首次探测到来自Ia型超新星 (SN Ia) 的无线电信号,揭示了富含的环恒星物质. 这一发现支持这些宇宙爆炸的单一退化原始模型.
科学领域:
- 天文学
- 天体物理学
- 宇宙学
背景情况:
- 一类超新星 (SNe Ia) 是重要的宇宙爆炸,但它们的原始系统在很大程度上是未知的.
- 无线电观测是区分原始模型的关键,因为非退化伴侣应该产生可检测的无线电同步发射.
- 之前对SNe Ia的无线电对应物进行的搜索都没有成功,
研究的目的:
- 通过寻找无线电辐射来研究SN Ia的原始系统.
- 通过光谱和红外分析来描述SN Ia的环恒星物质.
- 测试单一退化原始模型的Ia型超新星.
主要方法:
- 对SN 2020eyj进行了无线电观测.
- 分析了光谱特征和红外辐射以确定环恒星物质.
- 使用模型来解释环恒星物质的起源.
主要成果:
- 报告了第一个类型Ia超新星 (SN 2020eyj) 的无线电对应物.
- 在SN 2020eyj周围发现富含的环恒星物质.
- 根据观测到的无线电辐射和环恒星物质限制了原始系统.
结论:
- 检测到的无线电辐射和富含的环恒星物质支持SN 2020eyj的单一退化原始系统.
- 这一系统可能涉及白矮星从捐赠恒星中形成.
- 未来类似的SNe Ia的无线电追踪可以完善它们的原始来源的约束.
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