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Updated: Jul 20, 2026

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Absolute Quantum Yield Measurement of Powder Samples
Published on: May 12, 2012
巨大的恒星超新星作为主要的尘埃工厂
Ben E K Sugerman1, Barbara Ercolano, M J Barlow
1Space Telescope Science Institute, 3700 San Martin Drive, Baltimore, MD 21218, USA. sugerman@stsci.edu
概括
超新星喷射物中的尘埃形成在II型超新星2003gd.中观察到. 这表明大质量恒星是宇宙尘埃的重要生产者.
科学领域:
- 天文学 天文学
- 天体物理学 天体物理学
- 宇宙尘埃的形成
背景情况:
- 超新星对于将重元素分散到星际介质中至关重要.
- 超新星喷射中的尘埃形成是早期宇宙丰富的一个关键过程.
研究的目的:
- 为了研究二型超新星 (SN 2003gd) 的喷射物中的尘埃形成.
- 量化尘埃形成的数量和时间.
- 评估超新星作为产生尘埃的作用.
主要方法:
- 在SN 2003gd.的晚期光学和中红外观测.
- 分析中红外过量和光学灭绝.
- 辐射转移模型的应用.
主要成果:
- 观察到的中红外过量表明喷射物中的冷却尘埃 (喷发后499678天).
- 增加光学灭绝和排放线形状不对称.
- 辐射转移模型估计高达0.02太阳质量的尘埃早在爆发后250天就形成了.
结论:
- 超新星喷射中的尘埃形成可以非常高效.
- 巨大的恒星超新星可能是整个宇宙历史上宇宙尘埃产生的主要贡献者.
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