MWC 922の周りにある対称な双極星雲です
1Physics Department, University of Sydney, NSW 2006, Australia. p.tuthill@physics.usyd.edu.au
Science (New York, N.Y.)
|April 14, 2007
まとめ
赤外線画像は,粉塵に包まれたビー星MWC 922の周りの規則的で対称な構造を明らかにし",赤方形"の星雲を形成しています. この構造は,その独特な特徴で,混沌とした効果による最小限の障害を示唆しています.
科学分野:
- 天文学と天体物理学について
- 恒星の進化について
- ネブラー物理学 ネブラー物理学
背景:
- ビー星は,周周円盤を持つ,急速に回転するB型星である.
- 粉塵に覆われた星は,詳細な構造分析に課題をもたらす.
- MWC 922は,異常な周囲の星雲を持つ独特のビー星です.
研究 の 目的:
- ベー星MWC 922を囲む星雲の詳細な構造を調査する.
- 塵で覆われたオブジェクトの形態と対称性を分析するために.
- 観察された構造の形成機構を理解する.
主な方法:
- MWC 922の赤外線イメージング
- 星雲構造の形態学的分析. 星雲構造の形態学的分析.
- 既知の天体物理現象との比較.
主要な成果:
- MWC 922の周りの非常に規則的で対称な構造を発見し",赤方形"星雲と名付けました.
- ほぼ正方形の側面を持つ二角形の葉の観察,階段で交差し,明るい結び目で終わります.
- 双重ハイパーボリックアークと線形構造を形成する赤道暗帯の識別.
- 超新星1987A.の周辺のシステムと比べられるような,ノストした極環が観測されました.
結論:
- 複雑で明確に定義された構造は,地球規模の混乱や混沌の影響を最小限にすることを示唆しています.
- 線形の構造は,内側の円盤内の周期的な特徴を示す可能性があります.
- 観測された形態学は,ビー・スターの進化と質量放出過程の最終段階についての洞察を提供します.
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