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Fast and not-so-furious: Case study of the fast and faint Type IIb SN 2021bxu
dc.abstract.en | We present photometric and spectroscopic observations and analysis of SN 2021bxu (ATLAS21dov), a low-luminosity, fast-evolving Type IIb supernova (SN). SN 2021bxu is unique, showing a large initial decline in brightness followed by a short plateau phase. With $M_r = -15.93 pm 0.16, mathrm{mag}$ during the plateau, it is at the lower end of the luminosity distribution of stripped-envelope supernovae (SE-SNe) and shows a distinct ~10 d plateau not caused by H- or He-recombination. SN 2021bxu shows line velocities which are at least $sim 1500, mathrm{km, s^{-1}}$ slower than typical SE-SNe. It is photometrically and spectroscopically similar to Type IIb SNe during the photospheric phases of evolution, with similarities to Ca-rich IIb SNe. We find that the bolometric light curve is best described by a composite model of shock interaction between the ejecta and an envelope of extended material, combined with a typical SN IIb powered by the radioactive decay of <SUP>56</SUP>Ni. The best-fitting parameters for SN 2021bxu include a <SUP>56</SUP>Ni mass of $M_{mathrm{Ni}} = 0.029^{+0.004}_{-0.005}, mathrm{{ m M}_{odot }}$, an ejecta mass of $M_{mathrm{ej}} = 0.61^{+0.06}_{-0.05}, mathrm{{ m M}_{odot }}$, and an ejecta kinetic energy of $K_{mathrm{ej}} = 8.8^{+1.1}_{-1.0} imes 10^{49}, mathrm{erg}$. From the fits to the properties of the extended material of Ca-rich IIb SNe we find a trend of decreasing envelope radius with increasing envelope mass. SN 2021bxu has M<SUB>Ni</SUB> on the low end compared to SE-SNe and Ca-rich SNe in the literature, demonstrating that SN 2021bxu-like events are rare explosions in extreme areas of parameter space. The progenitor of SN 2021bxu is likely a low-mass He star with an extended envelope. |
dc.affiliation | Uniwersytet Warszawski |
dc.contributor.author | Desai, Dhvanil D. |
dc.contributor.author | Ashall, Chris |
dc.contributor.author | Shappee, Benjamin J. |
dc.contributor.author | Morrell, Nidia |
dc.contributor.author | Galbany, Lluís |
dc.contributor.author | Burns, Christopher R. |
dc.contributor.author | DerKacy, James M. |
dc.contributor.author | Hinkle, Jason T. |
dc.contributor.author | Hsiao, Eric |
dc.contributor.author | Kumar, Sahana |
dc.contributor.author | Lu, Jing |
dc.contributor.author | Phillips, Mark M. |
dc.contributor.author | Shahbandeh, Melissa |
dc.contributor.author | Stritzinger, Maximilian D. |
dc.contributor.author | Baron, Eddie |
dc.contributor.author | Bersten, Melina C. |
dc.contributor.author | Brown, Peter J. |
dc.contributor.author | Jaeger, Thomas de |
dc.contributor.author | Elias-Rosa, Nancy |
dc.contributor.author | Folatelli, Gastón |
dc.contributor.author | Huber, Mark E. |
dc.contributor.author | Mazzali, Paolo |
dc.contributor.author | Müller-Bravo, Tomás E. |
dc.contributor.author | Piro, Anthony L. |
dc.contributor.author | Polin, Abigail |
dc.contributor.author | Suntzeff, Nicholas B. |
dc.contributor.author | Anderson, Joseph P. |
dc.contributor.author | Chambers, Kenneth C. |
dc.contributor.author | Chen, Ting-Wan |
dc.contributor.author | Boer, Thomas de |
dc.contributor.author | Fulton, Michael D. |
dc.contributor.author | Gao, Hua |
dc.contributor.author | Gromadzki, Mariusz |
dc.contributor.author | Inserra, Cosimo |
dc.contributor.author | Magnier, Eugene A. |
dc.contributor.author | Nicholl, Matt |
dc.contributor.author | Ragosta, Fabio |
dc.contributor.author | Wainscoat, Richard |
dc.contributor.author | Young, David R. |
dc.date.accessioned | 2024-01-25T00:16:40Z |
dc.date.available | 2024-01-25T00:16:40Z |
dc.date.copyright | 2023-03-23 |
dc.date.issued | 2023 |
dc.description.accesstime | BEFORE_PUBLICATION |
dc.description.finance | Publikacja bezkosztowa |
dc.description.number | 1 |
dc.description.version | ORIGINAL_AUTHOR |
dc.description.volume | 524 |
dc.identifier.doi | 10.1093/MNRAS/STAD1932 |
dc.identifier.issn | 0035-8711 |
dc.identifier.uri | https://repozytorium.uw.edu.pl//handle/item/106996 |
dc.identifier.weblink | http://adsabs.harvard.edu/abs/2023MNRAS.524..767D |
dc.language | eng |
dc.pbn.affiliation | astronomy |
dc.relation.ispartof | Monthly Notices of the Royal Astronomical Society |
dc.relation.pages | 767-785 |
dc.rights | CC-BY |
dc.sciencecloud | nosend |
dc.title | Fast and not-so-furious: Case study of the fast and faint Type IIb SN 2021bxu |
dc.type | JournalArticle |
dspace.entity.type | Publication |