Last Updated:2025/12/06

The research team published a paper arguing that the observed Type Ia supernova was caused by a carbon detonation in a carbon-oxygen white dwarf following mass accretion from a companion star.

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The research team published a paper arguing that the observed Type Ia supernova was caused by a carbon detonation in a carbon-oxygen white dwarf following mass accretion from a companion star.

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研究チームは、観測されたIa型超新星が連星からの質量降着後に炭素と酸素からなる白色矮星で起きた炭素爆発(熱核融合の爆発的着火)によって引き起こされたと主張する論文を発表した。

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