Detached Circumstellar Matter as an Explanation for Slowly-Rising Interacting Type Ibc Supernovae

Autor:	Takei, Yuki, Tsuna, Daichi
Rok vydání:	2024
Předmět:	Astrophysics - High Energy Astrophysical Phenomena Astrophysics - Solar and Stellar Astrophysics
Druh dokumentu:	Working Paper
Popis:	Some hydrogen-poor (Type Ibc) supernovae (SNe) are known to have massive circumstellar matter (CSM) that are well detached from the star. Using the open-source code CHIPS, we construct a grid of models of SN Ibc interacting with detached CSM. We find that interaction with detached CSM can produce a slowly rising phase in the light curve seen in some interacting SN Ibc, which is difficult to reproduce by interaction with CSM of a density profile motivated from wind or eruptions that are continuous down to the star. We also show that SNe having double peaks in their light curves with timescales of months (e.g., SN 2022xxf) can be explained by radioactive decay of $^{56}$Ni/$^{56}$Co, followed by interaction with detached CSM. Comment: 8 pages, 4 figures, 1 table. To be submitted to The Open Journal of Astrophysics
Databáze:	arXiv
Externí odkaz:	http://arxiv.org/abs/2404.02566 Zobrazit plný text záznamu View this record from Arxiv