セントアウルスAの周りを回転する衛星銀河の平面は,冷たい暗黒物質の宇宙論に挑戦しています
Oliver Müller1, Marcel S Pawlowski2, Helmut Jerjen3
1Departement Physik, Universität Basel, Klingelbergstrasse 82, CH-4056 Basel, Switzerland. oliver89.mueller@unibas.ch.
まとめ
センタウルスA銀河の周りの衛星銀河は,薄い平面でのコロテーションの証拠を示しています. この発見は宇宙学的モデルに 異議を唱えていて 軌道上の衛星システムが 珍しいものではなく 共通点かもしれないことを示唆しています
科学分野:
- 天文学
- 天体物理学
- 宇宙学
背景:
- ミルクウェイとアンドロメダ銀河は 衛星矮星銀河の薄い平面を示し 潜在的に旋回しています
- これらのシステムは,宇宙学的なシミュレーションが同位衛星分布を予測しているため,しばしば稀な異常値と見なされます.
研究 の 目的:
- センタウルスA周辺の衛星銀河の動力学を調査する
- 衛星の回転が 統計的に珍しいという仮説を検証するためです
主な方法:
- センタウルスAを周回する16の衛星銀河の運動分析
- 観測された衛星運動と宇宙学的シミュレーションからの予測の統計的比較.
主要な成果:
- 狭い平面での回転の証拠は センタウルスAの衛星の間で発見された.
- 16の衛星のうち14の衛星は 空間分布に一致する一貫した速度パターンを示した.
- このような組織的な動きは,シミュレートされたCentaurus Aのようなシステムの0.5%未満で観察されます.
結論:
- 衛星銀河系は宇宙で一般的かもしれません
- コロテーションシステムの普及は,標準的な宇宙学的パラダイム内の小規模構造形成の現在のモデルに挑戦しています.
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