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巨大な宿主銀河を持たない明るいクワザーの発見
Pierre Magain1, Géraldine Letawe, Frédéric Courbin
1Institut d'Astrophysique et de Géophysique, Université de Liège, Allée du 6 Août, 17, Bât B5C, B-4000 Liège, Belgium. Pierre.Magain@ulg.ac.be
Nature
|September 16, 2005
まとめ
天文学者は,恒星のないガス雲の端にあるクエーサーを発見し,クエーサーの宿主銀河に関する以前の考え方に異議を唱えました. この発見は,クエーサーが,これまで考えられていたよりも明るさが低い環境で存在する可能性があることを示唆しています.
科学分野:
- 天文学と天体物理学について
- コスモロジー・コスモロジーとは
背景:
- クエザーは超大質量ブラックホールで動いているが,宿主銀河はクエザーの明るさのために研究するのが難しいことが多い.
- "裸"クワザーの存在は,1990年代に論争の的だった.
研究 の 目的:
- 新しく発見されたクエサールとその周辺環境の性質を調査するために.
- クワザールが典型的な宿主銀河と関連しているかどうかを判断する.
主な方法:
- 光学およびスペクトル分析を用いた観測天文学.
- クワザーの光度と潜在的宿主銀河の放射を比較する.
主要な成果:
- 小さな銀河のサイズに匹敵するガス雲の端にあるクエーサーの発見.
- ガス雲には恒星の痕跡がなく,クワザールによって興奮している.
- 潜在的な宿主銀河は,このような明るいクワザールに期待されるよりも少なくとも6倍弱くなっています.
結論:
- この発見は,すべての明るいクエサールが明るい宿主銀河に宿っているという仮定に異議を唱えている.
- クワザールは,隣の銀河と相互作用し,中央のブラックホールに潜在的に供給している可能性があります.
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