高赤位移転のクワサール内の塵のための超新星起源.
R Maiolino1, R Schneider, E Oliva
1INAF-Osservatorio Astrofisico di Arcetri, Firenze, Italy. maiolino@arcetri.astro.it
Nature
|October 1, 2004
まとめ
進化した星ではなく超新星は,宇宙初期に星間塵を形成した可能性が高い. 高赤偏移クエーサーの赤外線観測は,この超新星塵の起源理論を支持する.
科学分野:
- 宇宙塵の形成とは,宇宙塵の形成である.
- 初期の宇宙の天体物理学
- クワザーの進化とは
背景:
- 星間塵は分子や星形成に不可欠であり,吸収された光を再発する.
- 塵は,進化した低質量恒星で形成されると伝統的に考えられている.
- 初期のクエサールにおける塵の最近の発見は,この起源に異議を唱えている.
研究 の 目的:
- 初期の宇宙における塵の起源を調査する.
- 超新星が初期の宇宙塵を生成するという仮説を検証する.
主な方法:
- 赤外線観測 クワザーの赤外線観測 6.2.2.
- クワザールの塵の消滅曲線を直接決定する.
- 観測された絶滅曲線と理論上の超新星塵モデルを比較する.
主要な成果:
- 高赤偏移クワザーの塵の絶滅曲線は,超新星塵モデルと密接に一致しています.
- この合意は,超新星による塵の形成の直接的な証拠を提供する.
結論:
- 超新星は,高赤偏移クエーサーの星間塵の発生源である可能性が高い.
- 初期の宇宙のほとんどの塵はおそらく超新星から発生しています.
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