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双星分数为76%和NGC 188的蓝色落后者不寻常的轨道参数

Robert D Mathieu1, Aaron M Geller

  • 1Department of Astronomy, University of Wisconsin-Madison, 475 North Charter Street, Madison, Wisconsin 53706, USA. mathieu@astro.wisc.edu

Nature
|December 25, 2009
PubMed
概括

大多数蓝色滞留恒星都存在于二进制星系中,这表明它们不寻常的亮度和质量增长是多星系内部相互作用的结果. 这一发现有助于解决它们的形成途径.

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