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• W2004564101 abstract "Context. Core-collapse Supernovae (CC-SNe) descend from progenitors more massive than about 8 M⊙. Because of the young age of the progenitors, the ejecta may eventually interact with the circumstellar medium (CSM) via highly energetic processes detectable in the radio, X-ray, ultraviolet (UV) and, sometimes, in the optical domains." @default.
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• W2004564101 date "2013-07-01" @default.
• W2004564101 modified "2023-10-02" @default.
• W2004564101 title "Moderately luminous Type II supernovae" @default.
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• W2004564101 doi "https://doi.org/10.1051/0004-6361/201220496" @default.
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