Journal article
Probing Presupernova Mass Loss in Double-peaked Type Ibc Supernovae from the Zwicky Transient Facility
The Astrophysical journal, v 972(1), p91
01 Sep 2024
Abstract
<p>Eruptive mass loss of massive stars prior to supernova (SN) explosion is key to understanding their evolution and end fate. An observational signature of pre-SN mass loss is the detection of an early, short-lived peak prior to the radioactive-powered peak in the lightcurve of the SN. This is usually attributed to the SN shock passing through an extended envelope or circumstellar medium. Such an early peak is common for double-peaked Type IIb SNe with an extended hydrogen envelope but uncommon for normal Type Ibc SNe with very compact progenitors. In this paper, we systematically study a sample of 14 double-peaked Type Ibc SNe out of 475 Type Ibc SNe detected by the Zwicky Transient Facility. The rate of these events is similar to 3%-9% of Type Ibc SNe. A strong correlation is seen between the peak brightness of the first and the second peak. We perform a holistic analysis of this sample's photometric and spectroscopic properties. We find that six SNe have ejecta mass less than 1.5 M (circle dot). Based on the nebular spectra and lightcurve properties, we estimate that the progenitor masses for these are less than similar to 12 M- circle dot. The rest have an ejecta mass >2.4 M (circle dot) and a higher progenitor mass. This sample suggests that the SNe with low progenitor masses undergo late-time binary mass transfer. Meanwhile, the SNe with higher progenitor masses are consistent with wave-driven mass loss or pulsation-pair instability-driven mass-loss simulations.</p>
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Details
- Title
- Probing Presupernova Mass Loss in Double-peaked Type Ibc Supernovae from the Zwicky Transient Facility
- Creators
- Kaustav K. Das - California Institute of TechnologyMansi M. Kasliwal - California Institute of TechnologyJesper Sollerman - AlbaNovaChristoffer Fremling - California Institute of TechnologyI. Irani - Weizmann Institute of ScienceShing-Chi Leung - SUNY Polytechnic InstituteSheng Yang - Stockholm UniversitySamantha Wu - California Institute of TechnologyJim Fuller - California Institute of TechnologyShreya Anand - California Institute of TechnologyIgor Andreoni - Joint Space Science InstituteC. Barbarino - Stockholm UniversityThomas G. Brink - University of California, BerkeleyKishalay De - Kavli Institute for Particle Astrophysics and CosmologyAlison Dugas - University of Hawaii SystemSteven L. Groom - Infrared Processing and Analysis CenterGeorge Helou - Infrared Processing and Analysis CenterK-Ryan Hinds - Liverpool John Moores UniversityAnna Y. Q. Ho - Lawrence Berkeley National LaboratoryViraj Karambelkar - California Institute of TechnologyS. R. Kulkarni - California Institute of TechnologyDaniel A. Perley - Liverpool John Moores UniversityJosiah Purdum - California Institute of TechnologyNicolas Regnault - Laboratoire de Physique Nucléaire et de Hautes ÉnergiesSteve Schulze - AlbaNovaYashvi Sharma - California Institute of Technology Cahill Center for Astrophysics, MC 249-17, 1200 East California Boulevard, Pasadena, CA 91125, USATawny Sit - The Ohio State UniversityNiharika Sravan - Drexel UniversityGokul P. Srinivasaragavan - University of Maryland, College ParkRobert Stein - California Institute of TechnologyKirsty Taggart - University of California, Santa CruzLeonardo Tartaglia - Fraunhofer Chalmers Research Centre for Industrial MathematicsAnastasios Tzanidakis - California Institute of TechnologyAvery Wold - Infrared Processing and Analysis CenterLin Yan - California Institute of TechnologyYuhan Yao - California Institute of TechnologyJeffry Zolkower - California Institute of Technology
- Publication Details
- The Astrophysical journal, v 972(1), p91
- Publisher
- The American Astronomical Society; BRISTOL
- Number of pages
- 21
- Grant note
- 1545949 / National Science Foundation (NSF) (https://doi.org/10.13039/100000001) 1106171 / National Science Foundation (NSF) (https://doi.org/10.13039/100000001) 12540303 / Heising-Simons Foundation (HSF) (https://doi.org/10.13039/100014155)
- Resource Type
- Journal article
- Language
- English
- Academic Unit
- Physics
- Web of Science ID
- WOS:001299545000001
- Scopus ID
- 2-s2.0-85202564173
- Other Identifier
- 991021902314504721
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- Collaboration types
- Domestic collaboration
- International collaboration
- Web of Science research areas
- Astronomy & Astrophysics