ラジオ銀河のログ S-ログ z 図とその宇宙学との関係
1Institute of Theoretical Astronomy, University of Cambridge.
Nature
|July 25, 1970
まとめ
ラジオ銀河の流れと赤道移転に関するこの研究は,安定状態宇宙学モデルを支持している. 発見は,宇宙の連続的な創造論のさらなる調査を奨励しています.
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:
- 安定状態理論は,宇宙における物質の継続的な創造を提唱しています.
- ラジオ銀河は,その独特な特性により,宇宙学的モデルをテストする上で極めて重要です.
研究 の 目的:
- 安定状態宇宙学の実行可能性を評価する.
- ラジオ銀河におけるフクスとレッドシフトの関係を分析する.
主な方法:
- 第3のケンブリッジカタログのラジオ銀河データを調べました.
- これらの銀河の流れ (S) と赤道移転 (z) の分布を分析した.
主要な成果:
- ラジオ銀河の観測された流動-赤道移転関係は,安定状態モデルの予測と一致しています.
- データは,競合するモデルよりも安定状態の宇宙論を奨励しています.
結論:
- 安定状態宇宙論は,宇宙の合理的なモデルである.
- これらの発見を確認するために,さらなる観察データが必要である.
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