环恒星物质被一颗巨大的恒星在死亡前立即猛烈抛出.
Jujia Zhang1, Han Lin2, Xiaofeng Wang3
1Yunnan Observatories (YNAO), Chinese Academy of Sciences, Kunming 650216, China; Key Laboratory for the Structure and Evolution of Celestial Objects, Chinese Academy of Sciences, Kunming 650216, China; International Centre of Supernovae, Yunnan Key Laboratory, Kunming 650216, China.
Science bulletin
|September 24, 2023
概括
二型超新星很常见,但它们的祖先仍然是神秘的. 在SN 2023ixf中使用
科学领域:
- 天文学和天体物理学
- 恒星进化 恒星进化
- 超新星残留物 超新星残留物
背景情况:
- 第二类超新星是最常见的恒星爆炸.
- 它们巨大的,富含的祖先在核心崩之前的进化还不太清楚.
- 在Messier 101中SN 2023ixf提供了一个独特的机会来研究这些事件.
研究的目的:
- 研究大质量恒星的最后进化阶段,导致II型超新星.
- 通过早期观测来限制SN 2023ixf周围环恒星物质的特性.
- 为了确定SN 2023ixf.的祖先类型.
主要方法:
- 在爆炸后1-5天内分析SN 2023ixf的高频率闪光光谱.
- 监测狭窄的排放线快速消失的情况.
- 研究早期Hα发射的亮度和形状.
主要成果:
- 在爆炸前的最后2-3年,预计原始物质质量损失率约为6x10^-4 M/年.
- 探测到以~55公里/秒的速度移动的环恒星物质,形成一个7x10^14厘米的紧外.
- 爆炸前的观测表明,可能是黄色超巨人的祖先.
结论:
- SN 2023ixf的祖先在爆炸前不久经历了显著的质量损失.
- 这种祖先很可能从红色超巨型进化为短命的黄色超巨型.
- 这些发现为大质量恒星的最终演变提供了关键的见解.
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