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Updated: Jun 10, 2026

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Published on: February 12, 2013

タイコ・ブラヘの1572年の超新星は,その光エコースペクトルによって明らかにされる標準型Iaである

Oliver Krause1, Masaomi Tanaka, Tomonori Usuda

  • 1Max-Planck-Institut für Astronomie, Königstuhl 17, 69117 Heidelberg, Germany. krause@mpia.de

Nature
|December 5, 2008
PubMed
まとめ

研究者は,Tychoの超新星 (SN 1572) の光のエコーを分析した. この研究では,そのスペクトル型を決定し,それがこれらの宇宙爆発の通常のクラスに属していることを明らかにしました.

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