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Updated: Apr 15, 2026

Scattering And Absorption of Light in Planetary Regoliths
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若い恒星形成環境におけるタイプIア超新星からの距離は,<4%の精度で測定されます

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
まとめ

タイプIa超新星 (SNe Ia) の輝度は,その色と衰える速さと相関しています. 高紫外線環境でのSNe Iaの特定は,GALEXデータを用いて正確な距離校正 (<4%) を可能にし,その特性を支配するプライマリプロジェントプロパティを明らかにしました.

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