一个短暂的无线电源与核崩超新星相一致
D Z Dong1, G Hallinan1, E Nakar2
1Division of Physics, Mathematics, and Astronomy, California Institute of Technology, Pasadena, CA 91125, USA.
概括
我们发现了一个潜在的聚合驱动的超新星. 这一事件显示了早期的相对论喷射和晚期的相互作用,支持二进制诱导恒星爆炸的理论.
科学领域:
- 天体物理学
- 恒星进化
- 爆炸性短暂物质
背景情况:
- 核心崩超新星是巨大的恒星中核聚变停止的结果.
- 二元伴星的合并被认为会更早地中断核聚变,引发超新星.
- 无线电短暂提供了超新星喷射和相互作用环境的洞察力.
研究的目的:
- 报告发现和分析一个发光的无线电瞬态,VT J121001+495647.
- 研究二进制相互作用与超新星特征之间的潜在联系.
- 测试融合驱动的超新星爆炸的理论预测.
主要方法:
- 使用来自Very Large Array天空调查的数据来检测无线电短暂.
- 分析无线电辐射以推断超新星喷射物质和与周围物质的相互作用.
- 将无线传递器与存档X射线传递器关联起来以确定相对论喷气活动.
主要成果:
- 检测到一个发光的无线电瞬态,VT J121001+495647,
- 证据表明,在超新星发生之前,由二进制相互作用排出的物质存在密集的外.
- 在爆炸过程中发射了一颗相对论喷气.
结论:
- 观测到的无线电短暂和相关的X射线事件支持聚合驱动的超新星的假设.
- 早期相对论喷流与晚期密集相互作用的结合符合二进制引发爆炸的理论模型.
- 这一发现为核心崩的超新星提供了观测证据.
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