第二类超新星是星际尘埃的重要来源
Loretta Dunne1, Stephen Eales, Rob Ivison
1Department of Physics and Astronomy, Cardiff University, 5 The Parade, Cardiff CF24 3YB, UK. L.Dunne@astro.cf.ac.uk
Nature
|July 18, 2003
概括
超新星爆炸,而不仅仅是恒星风,是宇宙尘埃形成的关键. 这项研究在年轻的超新星残留物中发现了大量的尘埃,支持它们在早期星系进化中的作用.
科学领域:
- 天文学 天文学
- 天体物理学 天体物理学
- 宇宙尘埃研究 宇宙尘埃研究
背景情况:
- 高红移的类星体和星系含有大量的尘埃 (>10^8 M).
- 来自非对称的巨型分支恒星的恒星风不足以在所需的短时间尺度 (<1 Gyr) 上产生尘埃.
- 超新星 (II型) 被假设为来源,但对银河系残骸的观测显示尘埃有限 (10^-710^-3 M).
研究的目的:
- 为了研究超新星的尘埃产生能力.
- 为了协调超新星的理论尘埃产量与观测证据之间的差异.
主要方法:
- 观测已知最年轻的银河系超新星残留物,Cassiopeia A. 的观测.
- 在残留物中测量冷尘量.
主要成果:
- 在Cassiopeia A.中检测到大约24 M的冷尘.
- 这个数量远远超过了以前在超新星残骸中发现的尘埃.
结论:
- 超新星爆炸是银河系尘埃的主要来源,至少与恒星风一样重要.
- 超新星可能在早期宇宙中主导了尘埃的产生,解释了高红移尘埃的观测.
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