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Assembly of Complex Microtubule Structures
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非常に若い原星群のセルペンズ・サウスにおけるエピソード的分子流出
Adele L Plunkett1, Héctor G Arce1, Diego Mardones2
1Astronomy Department, Yale University, New Haven, Connecticut 06511, USA.
Nature
|November 6, 2015
まとめ
プロトステラ外流は,密集した星群の恒星形成の初期段階でも,エピソード的な質量放出現象を呈する. これはこれらの環境で星形成を制御する 重要な渦巻を供給します
科学分野:
- * 天文学と天体物理学
- * 星の形成と進化
- * プロトステラジェットと流出
背景:
- * 原星質量増はジェットや流出による質量減少に伴います.
- * エピソード的放出は,クラス0とクラスIの原星相で観察される.
- * 密集した恒星群の流出の振る舞いはよく理解されていません.
研究 の 目的:
- * クラスタ化された環境における若き原星からの蓄積による流出の性質を調査する.
- * 星団内の原始恒星の進化の初期段階でエピソード的放出イベントが発生するかどうかを決定する.
- * 原星群の運動量とエネルギーの移転における流出の役割を理解する.
主な方法:
- 蛇南原星群の中心にある若い0級原星の観測.
- * 流出エジェクタの特徴を特定するために (12) C(16) O (J=2-1) の排出を分析する.
- 落下と回転の動力学を研究するために,C ((18) Oエンベロープの放出を調べる.
主要な成果:
- * 原星からのエピソード的な流出エジェクションの明確な証拠が見つかりました.
- *22の異なる流出エジェクタ特徴が検出され,最も最近のものは最も高い速度を示しています.
- * 流出は1mm連続放射ピークから発生する双極葉を形成し,周囲のエンベロープはインフォールとローテーションを示しています.
結論:
- * 突発的,増殖による流出は,原星進化の初期段階から始まります.
- * 星系外流は不変であり,密集した環境の中で機能します.
- * これらの流出は,クラスタでの効率的なモメンタム転送を通じて,渦巻を駆動する上で重要な役割を果たしている可能性があります.
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