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一颗巨大的恒星在超新星爆炸前40天爆发
E O Ofek1, M Sullivan, S B Cenko
1Benoziyo Center for Astrophysics, Weizmann Institute of Science, 76100 Rehovot, Israel. eran@astro.caltech.edu
Nature
|February 8, 2013
概括
大质量恒星可以在爆炸为超新星之前失去大量的质量. 这项研究观察了超新星前的质量损失事件,证实了因果关系,并支持大质量恒星进化的波驱动脉冲模型.
科学领域:
- 天文学和天体物理学
- 恒星进化 恒星进化
- 超新星是指一个超新星.
背景情况:
- 据理论,大质量恒星在超新星爆炸之前会经历极端的质量损失事件.
- 关于超新星前质量损失和最终爆炸之间的直接因果关系的观测证据有限.
- 了解这种联系对于研究大质量恒星的最后进化阶段至关重要.
研究的目的:
- 为了确定超新星前的质量损失事件和随后的超新星爆炸之间的因果关系.
- 为了研究一个特定的超新星前质量损失事件的性质和特征.
- 测试预测这种现象的理论模型.
主要方法:
- 对IIn型超新星SN 2010mc (PTF 10tel) 的观测.
- 获取和分析光度和光谱数据.
- 在超新星爆炸前40天发生的质量损失事件的时间分析.
主要成果:
- 在SN 2010mc.c.之前40天检测出一个显著的质量损失事件.
- 事件的特征是能量爆发释放~10^-2太阳质量在~2,000公里/秒,与能量~6x10^47 erg.
- 观察到的爆发特性与波驱动脉冲模型的预测一致.
结论:
- 时间距离的近距离强烈地暗示了观测到的质量损失和超新星爆炸之间的因果关系.
- 这些发现支持波驱动脉冲模型作为大质量恒星中超新星前质量损失的解释.
- 这项研究为大质量恒星的最终进化阶段提供了新的见解,导致超新星.
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