,

M Nicholl1, S J Smartt, A Jerkstrand

  • 1Astrophysics Research Centre, School of Mathematics and Physics, Queen's University Belfast, Belfast BT7 1NN, UK. mnicholl03@qub.ac.uk

Nature
|October 18, 2013
PubMed
まとめ

2つの新しい超明るい超新星は,ペア不安定性モデルに挑戦しています. 観測結果から,磁石で動く爆発が,これらと類似の宇宙現象を説明できる可能性が示唆されており,対不安定性超新星が稀であることを示唆しています.

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