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Supernova Explosions inside Carbon-Oxygen Circumstellar Shells

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arxiv 1009.4353 v2 pith:WLG5TJ6B submitted 2010-09-22 astro-ph.HE

S.I.Blinnikov (1 , 2 , 3) , E.I.Sorokina (2 , 3)((1) ITEP , (2) SAI , (3) MPA) This is my paper · ORCID
classification astro-ph.HE
keywords supernovacircumstellarmodelsshellshellscarboncarbon-oxygencurves
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Motivated by a recent discovery of Supernova 2010gx and numerical results of Fryer et al.(2010), we simulate light curves for several type I supernova models, enshrouded by dense circumstellar shells, or "super-wind", rich in carbon and oxygen and having no hydrogen. We demonstrate that the most luminous events like SN2010gx can be explained by those models at moderate explosion energies (2-3) foe if the total mass of SN ejecta and a shell is (3-5) Msun and the radius of the shell is ~10^{16} cm.

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  1. SN 2023xgo: Helium-rich Type Icn or Carbon-Flash Type Ibn supernova?

    astro-ph.HE 2025-06 conditional novelty 6.0 of 10

    SN 2023xgo is a transitional Type Icn/Ibn supernova whose early carbon lines fade into helium lines, indicating a two-component circumstellar medium.

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