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Investigation of Early Plasma Evolution Induced by Ultrashort Laser Pulses
Published on: July 2, 2012
ミルクウェイ銀河の形成と初期の進化
1Astronomisches Institut der Universität Basel, Venusstrasse 7, CH-4102 Binningen, Switzerland. Roland.Buser@unibas.ch
まとめ
銀河系はおそらく120億年以上前に小さな銀河から形成された. 衛星銀河の合併は,その独特の厚くて薄い円盤の発展に影響を与えた.
科学分野:
- 天文学と天体物理学について
- コスモロジー・コスモロジーとは
- 銀河の進化について
背景:
- 最近の観測により,天の川の形成には,より小さな銀河の増殖が伴うことが示唆されています.
- 初期の宇宙には,銀河の構造に貢献したガスと星の貯蔵庫がありました.
研究 の 目的:
- ミルクウェイ銀河の形成過程を明らかにするために.
- 衛星銀河の合併が銀河の構成要素を形成する役割を理解するために.
主な方法:
- 銀河の構造と構成に関する観測データの分析.
- 銀河の形成と進化をモデル化した宇宙学的シミュレーション.
主要な成果:
- 銀河系はおそらく120億年以上前に小さな銀河の集合によって形成された.
- 初期の物質の異なる角運動量は,ハロー/膨らみと円盤の異なる進化の経路につながった.
- 厚くて薄い円盤は,衛星銀河の合併が進行中であり,初期の進化に影響を与えたことを示しています.
結論:
- 銀河系の構造は,原始的な構成要素からヒエラルキーな組み立ての産物です.
- 衛星銀河の合併は,銀河系の主な構造的構成要素を確立する上で重要な役割を果たしました.
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