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Luminous Type II Short-Plateau Supernovae 2006Y, 2006ai, and 2016egz: A Transitional Class from Stripped Massive Red Supergiants
cris.lastimport.scopus | 2024-02-12T20:54:43Z |
dc.abstract.en | The diversity of Type II supernovae (SNe II) is thought to be driven mainly by differences in their progenitor's hydrogen-rich (H-rich) envelope mass, with SNe IIP having long plateaus (∼100 days) and the most massive H-rich envelopes. However, it is an ongoing mystery why SNe II with short plateaus (tens of days) are rarely seen. Here, we present optical/near-infrared photometric and spectroscopic observations of luminous Type II short-plateau SNe 2006Y, 2006ai, and 2016egz. Their plateaus of about 50-70 days and luminous optical peaks (≲-18.4 mag) indicate significant pre-explosion mass loss resulting in partially stripped H-rich envelopes and early circumstellar material (CSM) interaction. We compute a large grid of MESA+STELLA single-star progenitor and light-curve models with various progenitor zero-age main-sequence (ZAMS) masses, mass-loss efficiencies, explosion energies, <SUP>56</SUP>Ni masses, and CSM densities. Our model grid shows a continuous population of SNe IIP-IIL-IIb-like light-curve morphology in descending order of H-rich envelope mass. With large <SUP>56</SUP>Ni masses (≳0.05 M<SUB>⊙</SUB>), short-plateau SNe II lie in a confined parameter space as a transitional class between SNe IIL and IIb. For SNe 2006Y, 2006ai, and 2016egz, our findings suggest high-mass red supergiant (RSG) progenitors (M<SUB>ZAMS</SUB> ≃ 18-22 M<SUB>⊙</SUB>) with small H-rich envelope masses ( ${M}_{{{\rm{H}}}_{\mathrm{env}}}\simeq 1.7\,{M}_{\odot }$ ) that have experienced enhanced mass loss ( $\dot{M}\simeq {10}^{-2}\,{M}_{\odot }\,{\mathrm{yr}}^{-1}$ ) for the last few decades before the explosion. If high-mass RSGs result in rare short-plateau SNe II, then these events might ease some of the apparent underrepresentation of higher-luminosity RSGs in observed SN II progenitor samples. |
dc.affiliation | Uniwersytet Warszawski |
dc.contributor.author | Hiramatsu, Daichi |
dc.contributor.author | Howell, D. Andrew |
dc.contributor.author | Moriya, Takashi J. |
dc.contributor.author | Goldberg, Jared A. |
dc.contributor.author | Hosseinzadeh, Griffin |
dc.contributor.author | Arcavi, Iair |
dc.contributor.author | Anderson, Joseph P. |
dc.contributor.author | Gutiérrez, Claudia P. |
dc.contributor.author | Burke, Jamison |
dc.contributor.author | McCully, Curtis |
dc.contributor.author | Valenti, Stefano |
dc.contributor.author | Galbany, Lluís |
dc.contributor.author | Fang, Qiliang |
dc.contributor.author | Maeda, Keiichi |
dc.contributor.author | Folatelli, Gastón |
dc.contributor.author | Hsiao, Eric Y. |
dc.contributor.author | Morrell, Nidia I. |
dc.contributor.author | Phillips, Mark M. |
dc.contributor.author | Stritzinger, Maximilian D. |
dc.contributor.author | Suntzeff, Nicholas B. |
dc.contributor.author | Gromadzki, Mariusz |
dc.contributor.author | Maguire, Kate |
dc.contributor.author | Müller-Bravo, Tomás E. |
dc.contributor.author | Young, David R. |
dc.date.accessioned | 2024-01-25T05:29:55Z |
dc.date.available | 2024-01-25T05:29:55Z |
dc.date.copyright | 2020-10-29 |
dc.date.issued | 2021 |
dc.description.accesstime | BEFORE_PUBLICATION |
dc.description.finance | Publikacja bezkosztowa |
dc.description.number | 1 |
dc.description.version | ORIGINAL_AUTHOR |
dc.description.volume | 913 |
dc.identifier.doi | 10.3847/1538-4357/ABF6D6 |
dc.identifier.issn | 0004-637X |
dc.identifier.uri | https://repozytorium.uw.edu.pl//handle/item/111600 |
dc.identifier.weblink | http://adsabs.harvard.edu/abs/2021ApJ...913...55H |
dc.language | eng |
dc.pbn.affiliation | astronomy |
dc.relation.ispartof | Astrophysical Journal |
dc.relation.pages | 55 |
dc.rights | Other |
dc.sciencecloud | nosend |
dc.title | Luminous Type II Short-Plateau Supernovae 2006Y, 2006ai, and 2016egz: A Transitional Class from Stripped Massive Red Supergiants |
dc.type | JournalArticle |
dspace.entity.type | Publication |