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背景の星光の消滅から推論された,冷たい暗い分子雲の内部構造
Nature
|February 24, 2001
まとめ
研究者は,近赤外線を用いて,暗い分子雲であるバーナード68を研究した. 彼らはその密度を正確にマッピングし,恒星形成に適した条件を明らかにした.
科学分野:
- 天文学と天体物理学について
- スター・フォーメーション
- 星間媒介は,星間媒介である.
背景:
- 星と惑星の形成は,暗い分子雲に由来する.
- これらの雲の内部構造と恒星形成の初期条件は,まだ十分に理解されていない.
- 主要な雲の構成要素である分子水素は,直接観測するのは困難です.
研究 の 目的:
- ダーククラウドバーナード68の内部構造を詳細に調査する.
- 恒星形成の瀬戸際にある暗い雲の中の物理的条件を理解するために.
主な方法:
- 繊細な近赤外線測定を用いた.
- 背景の星からの光が塵によって吸収され,散らばった.
- ガス特性を推測するために,塵の分布を調査した.
主要な成果:
- バーナード68の密度構造は,極めて安定した同熱球のモデルによって正確に記述されています.
- 雲は,圧力の収束と自己重力のボナー・エバート基準に準拠しています.
- 雲の中の正確な物理的条件が決定されました.
結論:
- バーナード68のような暗い雲は,塵の性質と近赤外線観測を使用して正確に研究することができます.
- この発見は,恒星の崩壊に必要な条件の詳細な理解を提供します.
- この研究は,星と惑星の形成の初期段階についての洞察を提供します.
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