銀河間媒体の低密度地域における重元素の濃縮
1Institute for Astronomy, University of Hawaii, Honolulu 96822, USA. cowie@uhifa.ifa.hawaii.edu
Nature
|July 17, 1998
まとめ
初期の銀河は予想外にも低密度の銀河間ガスを重元素で豊かにした. この発見は,宇宙化学進化のモデルに異議を唱え,小さな銀河が効率的に銀河間媒介に元素を放出したと示唆しています.
科学分野:
- コスモロジー・コスモロジーとは
- 天体物理学 天体物理学
- 銀河間媒介は銀河間媒介である.
背景:
- 宇宙学的モデルは,高赤偏移の低密度の銀河間ガスが元素に乏しいことを予測しています.
- 重元素の合成と分布は,密度の高い地域で優先的に発生すると考えられている.
研究 の 目的:
- 赤いシフト3で低密度の銀河間ガスの重元素の豊富さを探知する.
- クワザールスペクトルの炭素と酸素の吸収線を分析する.
主な方法:
- クワザールスペクトルの吸収線を分析する新しい方法を開発した.
- 炭素と酸素の吸収線を中心に重元素の豊富さを測定する.
- 密度範囲の範囲で,ゼロに近い密度領域を含むガスを調べました.
主要な成果:
- 三重イオン化された炭素と中性水素の比率は,密度によって相対的に一定でした.
- 密度がほぼゼロの地域でも,重元素の豊富さは予想外にも高かった.
- これは,低密度の銀河間ガスの濃縮が顕著であることを示している.
結論:
- 初期の小さな銀河は,重元素を銀河間媒質に放出するのに非常に効率的かもしれません.
- 銀河間媒体の組成に関する現在のモデルは,改定する必要があるかもしれない.
- 初期の宇宙の化学的濃縮過程の改訂された理解を示唆しています.
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