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Updated: Jul 7, 2026
11:59
High-speed Particle Image Velocimetry Near Surfaces
Published on: June 24, 2013
ラジオ銀河の分布における速度二極体
1Astrophysics, Nuclear and Astrophysics Laboratory, University of Oxford, UK. cab@astro.ox.uk
Nature
|March 15, 2002
まとめ
私たちの銀河系です.
科学分野:
- コスモロジー・コスモロジーとは
- 天体物理学 天体物理学
背景:
- 銀河系が宇宙を通る動きは,宇宙マイクロ波背景放射のドップラーシフトを引き起こし,二極アニソトロピーを生み出します.
- 遠い銀河の分布における同様の二極アニソトロピーは,標準宇宙学モデルによって予測されています.
研究 の 目的:
- 遠い銀河の分布における予測された宇宙学的な二極アニソトロピーを検出するために.
- 宇宙マイクロ波背景放射の標準的な宇宙学的解釈を確認するために.
主な方法:
- 主に宇宙学的距離で,ラジオ銀河の調査を利用した.
- 近くの銀河団からの汚染を最小限に抑えるために,サンプルからローカルなラジオ銀河を取り除きました.
主要な成果:
- 遠くのラジオ銀河の分布における二極アニソトロピーを検出しました.
- 検出された二極は,方向と振幅で宇宙マイクロ波背景二極アニソトロピーと一致します.
結論:
- この発見は,銀河分布における宇宙的二極アニソトロピーの証拠を提供する.
- この結果は,標準宇宙論モデルとその宇宙マイクロ波背景の解釈を裏付けている.
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