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Updated: Jul 7, 2026

Surface Mapping of Earth-like Exoplanets using Single Point Light Curves
06:48

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超新星爆発におけるアスフェリック性は,時代遅れのスペクトロスコピーによるものです.

Keiichi Maeda1, Koji Kawabata, Paolo A Mazzali

  • 1Institute for the Physics and Mathematics of the Universe (IPMU), University of Tokyo, Kashiwa-no-ha 5-1-5, Kashiwa City, Chiba 277-8582, Japan. maeda@ea.c.u-tokyo.ac.jp

Science (New York, N.Y.)
|February 2, 2008
PubMed
まとめ

剥離されたエンベロープの恒星からのほとんどのコア崩壊超新星 (CC-SNe) は,非対称な爆発の兆候を示しています. ガンマ線爆発 (GRB) に関連しているものは,最も顕著な非対称性を示します.

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