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Scattering And Absorption of Light in Planetary Regoliths
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在年轻恒星形成环境中的Ia型超新星距离精度<4%

Patrick L Kelly1, Alexei V Filippenko2, David L Burke3

  • 1Department of Astronomy, University of California, Berkeley, CA 94720-3411, USA. pkelly@astro.berkeley.edu.

Science (New York, N.Y.)
|March 28, 2015
PubMed
概括

类型Ia超新星 (SNe Ia) 的亮度与它们的颜色和色速度相关. 在高紫外线环境中使用 GALEX 数据识别 SNe Ia 允许精确的距离校准 (<4%),揭示一个主要的祖先属性支配它们的特征.

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