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  LSQ13ddu: a rapidly evolving stripped-envelope supernova with early circumstellar interaction signatures

Clark, P., Maguire, K., Inserra, C., Prentice, S., Smartt, S. J., Contreras, C., et al. (2020). LSQ13ddu: a rapidly evolving stripped-envelope supernova with early circumstellar interaction signatures. Monthly Notices of the Royal Astronomical Society, 492(2), 2208-2228. doi:10.1093/mnras/stz3598.

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Item Permalink: http://hdl.handle.net/21.11116/0000-0006-41F7-A Version Permalink: http://hdl.handle.net/21.11116/0000-0006-41F8-9
Genre: Journal Article

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 Creators:
Clark, Peter, Author
Maguire, Kate, Author
Inserra, Cosimo, Author
Prentice, Simon, Author
Smartt, Stephen J., Author
Contreras, Carlos, Author
Hossenizadeh, Griffin, Author
Hsiao, Eric Y., Author
Kankare, Erkki, Author
Kasliwal, Mansi, Author
Nugent, Peter, Author
Shahbandeh, Melissa, Author
Baltay, Charles, Author
Rabinowitz, David, Author
Arcavi, Iair, Author
Ashall, Chris, Author
Burns, Christopher R., Author
Callis, Emma, Author
Chen, Ting-Wan1, Author              
Diamond, Tiara, Author
Fraser, Morgan, AuthorHowell, D. Andrew, AuthorKaramehmetoglu, Emir, AuthorKotak, Rubina, AuthorLyman, Joseph, AuthorMorrell, Nidia, AuthorPhillips, Mark, AuthorPignata, Giuliano, AuthorPursiainen, Miika, AuthorSollerman, Jesper, AuthorStritzinger, Maximilian, AuthorSullivan, Mark, AuthorYoung, David, Author more..
Affiliations:
1High Energy Astrophysics, MPI for Extraterrestrial Physics, Max Planck Society, ou_159890              

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 Abstract: This paper describes the rapidly evolving and unusual supernova LSQ13ddu, discovered by the La Silla-QUEST survey. LSQ13ddu displayed a rapid rise of just 4.8 ± 0.9 d to reach a peak brightness of −19.70 ± 0.02 mag in the LSQgr band. Early spectra of LSQ13ddu showed the presence of weak and narrow [Math Processing Error] features arising from interaction with circumstellar material (CSM). These interaction signatures weakened quickly, with broad features consistent with those seen in stripped-envelope SNe becoming dominant around two weeks after maximum. The narrow [Math Processing Error] velocities are consistent with the wind velocities of luminous blue variables but its spectra lack the typically seen hydrogen features. The fast and bright early light curve is inconsistent with radioactive 56Ni powering but can be explained through a combination of CSM interaction and an underlying 56Ni decay component that dominates the later time behaviour of LSQ13ddu. Based on the strength of the underlying broad features, LSQ13ddu appears deficient in He compared to standard SNe Ib.

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 Dates: 2020-01-03
 Publication Status: Published online
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 Rev. Method: Peer
 Identifiers: DOI: 10.1093/mnras/stz3598
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Title: Monthly Notices of the Royal Astronomical Society
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Source Genre: Journal
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Publ. Info: OXFORD : OXFORD UNIV PRESS
Pages: - Volume / Issue: 492 (2) Sequence Number: - Start / End Page: 2208 - 2228 Identifier: ISSN: 0035-8711
CoNE: https://pure.mpg.de/cone/journals/resource/1000000000021470