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オリオン星座の分子雲の表面にある波
Olivier Berné1, Núria Marcelino, José Cernicharo
1Centro de Astrobiología, CSIC/INTA, Carretera de Torrejón a Ajalvir, km 4, 28850 Torrejón de Ardoz, Spain. berne@strw.leidenuniv.nl
Nature
|August 21, 2010
まとめ
天文学者はオリオン星座の分子雲の表面で波のような構造を発見し,水力学的不安定性の最初の証拠を提供した. これらの波は,巨大な恒星からの恒星風によって引き起こされるケルビン・ヘルムホルツの不安定性である可能性が高い.
科学分野:
- 天体物理学 天体物理学
- 水力ダイナミクスとは
- スター・フォーメーション
背景:
- 巨大な恒星は,周囲の分子雲に著しく影響を及ぼします.
- 水力学的不安定性は,雲の圧縮と断片化の原因であると疑われています.
- "創造の柱"のような雲の構造に関する以前の説明は,依然として議論の余地があります.
研究 の 目的:
- 分子雲の水力動力学的不安定性を特定し,特徴づけること.
- これらの不安定性のサインとして,波のような構造の観測的証拠を見つけること.
主な方法:
- オリオン星座の分子雲をターゲットにした観測天文学.
- 巨大な恒星形成地域近くのガス構造の分析.
主要な成果:
- オリオンの分子雲の表面に"波"の存在が検出されました.
- これらの波は,ケルビン・ヘルムホルツ不安定の潜在的サインとして識別されています.
- 不安定は,膨張する星雲ガスが,以前に存在していた分子ガスとの相互作用によって生じる.
結論:
- 観測された波は,分子雲における水力学的不安定性の最初の直接的な証拠を提供します.
- この発見は,恒星の活動が不安定性を通じた雲の進化を促すという理論を支持している.
- この発見は,星形成の複雑なプロセスに関する新しい洞察を提供します.
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