11 億 年 前 に 大 規模 な 銀河 を 囲っ て 観測 さ れ た 刺激 的 な ガス の 流れ
Shiwu Zhang1, Zheng Cai1,2, Dandan Xu1
1Department of Astronomy, Tsinghua University, Beijing 100084, China.
まとめ
ガスのリサイクルが 初期の恒星形成を促します 科学者は巨大な銀河の周りのガスの流れを観察し,以前に放出された物質の証拠を発見し,銀河の組立モデルを支持しました.
科学分野:
- 宇宙の進化
- 銀河の形成 と 進化
- 天体物理学
背景:
- 銀河の進化には 恒星形成が不可欠です
- シミュレーションによると ガス再利用は 恒星形成の維持に不可欠です 特に初期の宇宙では
- 銀河の形成の鍵となるものです 銀河の形成の鍵となるものです 銀河の形成の鍵となるものです
研究 の 目的:
- 高赤偏移の巨大な銀河の ガス循環を調査する
- 以前から放出されたガスの再形成の観測的証拠を提供すること.
- 初期の宇宙の星形成を 維持するメカニズムを理解する
主な方法:
- 赤い偏移2.3の巨大な銀河の観測
- ニュートラルな水素,ヘリウム,および銀河周りの環境でイオン化された炭素からの放射線の検出.
- 環銀河ガスの動力学と化学の分析
主要な成果:
- 放射線は銀河から 100キロパルセックまで検出されました
- 銀河の周りのガスの動力学は 吸気流と一致する
- 炭素の豊富さは,以前に放出された物質からの濃縮を示しています.
結論:
- 観測されたガス流は,ガスリサイクルの証拠として解釈されます.
- このリサイクルプロセスは,高赤偏移の銀河の集合の間に恒星形成の持続に貢献します.
- この発見は ガス循環を含む銀河進化の理論モデルを 支持しています
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