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Updated: May 5, 2026

Investigation of Early Plasma Evolution Induced by Ultrashort Laser Pulses
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Published on: July 2, 2012

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円銀河の珍しいヘリウム豊富な超新星のための巨大な星の起源

K S Kawabata1, K Maeda, K Nomoto

  • 1Hiroshima Astrophysical Science Center, Hiroshima University, 1-3-1 Kagamiyama, Higashi-Hiroshima, Hiroshima 739-8526, Japan. kawabtkj@hiroshima-u.ac.jp

Nature
|May 21, 2010
PubMed
まとめ

SN 2005czの超新星は,SN 2005Eに似ているが,低質量星の核崩壊による起源を示唆している. これは,異常な超新星に関する白矮星爆発理論に異議を唱える.

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