一个超新星起源的尘埃在一个高红移的类星体
R Maiolino1, R Schneider, E Oliva
1INAF-Osservatorio Astrofisico di Arcetri, Firenze, Italy. maiolino@arcetri.astro.it
Nature
|October 1, 2004
概括
超新星,而不是进化的恒星,可能在早期宇宙中形成星际尘埃. 一个高红移类星的红外观测支持了这种超新星尘埃起源理论.
科学领域:
- 宇宙尘埃的形成
- 早期宇宙的天体物理学
- 量子星的演化过程
背景情况:
- 星际尘埃对分子和恒星形成至关重要,并重新发射吸收的光.
- 传统上,人们认为尘埃是在进化的低质量恒星中形成的.
- 最近在早期类星体中发现的尘埃挑战了这个起源.
研究的目的:
- 在早期宇宙中调查尘埃的起源.
- 测试超新星产生早期宇宙尘埃的假设.
主要方法:
- 在红移6.2.2.2.的类星体的红外观测.
- 直接确定类星体的尘埃灭绝曲线.
- 将观察到的灭绝曲线与理论上的超新星尘埃模型进行比较.
主要成果:
- 高红移类星的尘埃灭绝曲线与超新星尘埃模型密切匹配.
- 这项协议提供了通过超新星形成尘埃的直接证据.
结论:
- 超新星是高红移类星体中星际尘埃的可能来源.
- 早期宇宙中的大部分尘埃可能起源于超新星.
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