银河系表面密度的普遍性在一个暗光环尺度-长度范围内
Gianfranco Gentile1, Benoit Famaey, HongSheng Zhao
1Sterrenkundig Observatorium, Universiteit Gent, Krijgslaan 281, B-9000 Gent, Belgium. gianfranco.gentile@ugent.be
Nature
|October 2, 2009
概括
星系在它们的暗光环尺度长度内显示出一致的发光物质表面密度. 这一发现揭示了星系中发光物质和暗物质分布之间的强烈相关性.
科学领域:
- 银河系天文学 银河系天文学
- 宇宙学的宇宙学是什么?
- 天体物理学 天体物理学
背景情况:
- 最近的研究显示,在各种星系的暗光环尺度长度内,暗物质表面密度的平均值是恒定的.
- 这种暗物质缩放关系适用于14级光度范围内的星系和整个哈勃测量序列.
研究的目的:
- 为了研究暗光环尺度长度内的发光物质的表面密度.
- 为了确定是否存在类似的恒定存在于发光物质和观察到的黑暗物质.
主要方法:
- 对星系中发光物质的表面密度概况的分析.
- 照亮物质表面密度与暗物质表面密度在光环尺度长度内的比较.
主要成果:
- 发光物质表面密度在一个暗光环尺度长度内也是恒定的.
- 发光物质的引力加速在这种特征半径上是均的.
- 虽然总亮度与暗度的物质比率有所变化,但在这个特定的光环尺度长度内是恒定的.
结论:
- 银河系中明亮和暗物质的封闭表面密度之间存在显著的相关性.
- 这些发现表明,银河系光环中的物质分布存在着根本关系.
- 这种常数为星系形成和进化模型提供了新的见解.
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