无线电星系的log S-log z图及其与宇宙学的关系
1Institute of Theoretical Astronomy, University of Cambridge.
Nature
|July 25, 1970
概括
这种对无线电星系流量和红移的研究支持了稳定状态宇宙学模型. 这些发现鼓励进一步研究宇宙的连续创造理论.
科学领域:
- 宇宙学的宇宙学是什么?
- 天体物理学 天体物理学
背景情况:
- 稳态理论提出宇宙中物质的持续创造.
- 无线电星系对于测试宇宙学模型至关重要,因为它们具有独特的特性.
研究的目的:
- 评估稳定状态宇宙学的可行性.
- 分析无线电星系中流量和红移之间的关系.
主要方法:
- 检查了来自第三个剑桥目录的无线电星系数据.
- 分析了这些星系的流量 (S) 和红移 (z) 分布.
主要成果:
- 观测到的射电星系的流量-红移关系与稳定状态模型的预测保持一致.
- 数据为稳定状态宇宙学提供了鼓励,而不是竞争模型.
结论:
- 恒定状态宇宙学仍然是宇宙的可信模型.
- 需要进一步的观察数据来证实这些发现.
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