近くの恒星AU Microscopiiの周りの大きな塵の円盤を発見した
Paul Kalas1, Michael C Liu, Brenda C Matthews
1Astronomy Department and Radio Astronomy Laboratory, 601 Campbell Hall, Berkeley, CA 94720, USA. kalas@astro.berkeley.edu
まとめ
天文学者は,若いM型恒星AU Microscopiiの周りを回る環状塵の円盤を発見した. この発見は,銀河系で最も一般的なタイプの星の周りの惑星形成の洞察を提供します.
科学分野:
- 天文学 (astronomy) 天文学 (astronomy) とは,天文学 (astronomy) とは,天文学 (astronomy) とは,天文学 (astronomy) とは
- 惑星外科学とは,惑星外科学です.
背景:
- AU Microscopii (AU Mic) は,若いM型恒星である.
- M型星は,銀河系で最も一般的な恒星型です.
- ベータ・ピクトリス (Beta Pictoris) は同様の若い星で,既知の塵の円盤がある.
研究 の 目的:
- AU Microscopii.の周りの周回恒星塵円盤の発見を報告するために.
- M型星の周りの惑星形成の可能性を調査する.
主な方法:
- 星周塵ディスクの直接観測.
主要な成果:
- AU Microscopii.の周りに円周塵ディスクが検出されました.
- 円盤は50から210の天文単位 (AU) に及ぶ.
- 円盤の中の塵は,恒星の現在の年齢よりも長い寿命を持っています.
結論:
- AU Microscopiiは,惑星形成のための直接観測された固体物質を持つ最も近い恒星です.
- AU Micディスクは,M型恒星系における惑星形成を理解するための重要なデータを提供します.
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