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銀河外流の内部で星が形成される
R Maiolino1,2, H R Russell3, A C Fabian3
1Cavendish Laboratory, University of Cambridge, 19 J. J. Thomson Avenue, Cambridge CB3 0HE, UK.
Nature
|March 28, 2017
まとめ
恒星形成の直接的な証拠を発見しました 巨大な銀河の流れの中で発生しています この発見は 銀河の進化に影響を及ぼし 銀河間媒体を豊かにする 恒星形成の新たな方法を示唆しています
科学分野:
- 天文学と天体物理学
- 銀河の進化
- 星の形成
背景:
- 巨大な銀河の流れは 恒星形成に有利な条件を持っています
- モデルでは 銀河の形態と星群に 影響を与える 流出中の星形成を予測しています
- 流出中の恒星形成の観測証拠は現在不足している.
研究 の 目的:
- 銀河の流れの中で 恒星形成の 明確な観測証拠を提供するためです
- 銀河の進化と化学的濃縮に 与える影響を調査する
主な方法:
- 赤道偏移0.0448で 銀河の流出を観測した
- 進行中の星形成のサインを特定するためにスペクトルデータを分析します.
主要な成果:
- 観測された銀河外流の星形成の 明確な検出
- 流出中の恒星形成率は 年間15太陽質量を超えています
- 過去の観測では 診断が不適切だったため 類似の現象が 見逃されたと示唆しています
結論:
- 恒星形成は 銀河の流出の中で起こり 前の仮定に異議を唱えます
- この星形成の様式は銀河の進化と 環銀河と銀河間媒体の化学的濃縮に 重要な役割を果たす可能性がある.
- 銀河の流出における星形成の頻度を評価するために,適切な診断を用いたさらなる観測が必要である.
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