Superluminous supernova SN 2018ibb: Circumstellar shell and spectral effects

Fuente: arXiv
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Autore principale: Chugai, Nikolai N.
Natura: Preprint
Pubblicazione: 2024
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author Chugai, Nikolai N.
author_facet Chugai, Nikolai N.
contents I explore observational effects of the cirsumstellar gas around superluminous supernova SN~2018ibb. High velocity Fe II narrow absorptions are reproduced in the model of fragmented cold dense shell. Unusual selective absorption in the emission doublet of [O I] is explained as an effect of the radiation scattering in Si II doublet lines in the supernova envelope.The strong emission of [O III] doublet at t_max + 565 days is proposed to originate from the supernova envelope, whereas its asymmetry is explained by the dust formation in the unshocked ejecta. Circumstellar interaction modeling combined with observational data suggests the cirsumstellar shell mass of about 0.14 Msun.
format Preprint
id arxiv_https___arxiv_org_abs_2410_17580
institution arXiv
publishDate 2024
record_format arxiv
spellingShingle Superluminous supernova SN 2018ibb: Circumstellar shell and spectral effects
Chugai, Nikolai N.
High Energy Astrophysical Phenomena
I explore observational effects of the cirsumstellar gas around superluminous supernova SN~2018ibb. High velocity Fe II narrow absorptions are reproduced in the model of fragmented cold dense shell. Unusual selective absorption in the emission doublet of [O I] is explained as an effect of the radiation scattering in Si II doublet lines in the supernova envelope.The strong emission of [O III] doublet at t_max + 565 days is proposed to originate from the supernova envelope, whereas its asymmetry is explained by the dust formation in the unshocked ejecta. Circumstellar interaction modeling combined with observational data suggests the cirsumstellar shell mass of about 0.14 Msun.
title Superluminous supernova SN 2018ibb: Circumstellar shell and spectral effects
topic High Energy Astrophysical Phenomena
url https://arxiv.org/abs/2410.17580