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

Clark, Peter (author)
Maguire, Kate (author)
Inserra, Cosimo (author)
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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-Wan (author)
Diamond, Tiara (author)
Fraser, Morgan (author)
Howell, D. Andrew (author)
Karamehmetoglu, Emir (author)
Stockholms universitet,Institutionen för astronomi,Oskar Klein-centrum för kosmopartikelfysik (OKC)
Kotak, Rubina (author)
Lyman, Joseph (author)
Morrell, Nidia (author)
Phillips, Mark (author)
Pignata, Giuliano (author)
Pursiainen, Miika (author)
Sollerman, Jesper (author)
Stockholms universitet,Institutionen för astronomi,Oskar Klein-centrum för kosmopartikelfysik (OKC)
Stritzinger, Maximilian (author)
Sullivan, Mark (author)
Young, David (author)
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 (creator_code:org_t)
2020-01-03
2020
English.
In: Monthly notices of the Royal Astronomical Society. - : Oxford University Press (OUP). - 0035-8711 .- 1365-2966. ; 492:2, s. 2208-2228
  • Journal article (peer-reviewed)
Abstract Subject headings
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  • 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 He I 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 He I 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 Ni-56 powering but can be explained through a combination of CSM interaction and an underlying Ni-56 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.

Subject headings

NATURVETENSKAP  -- Fysik (hsv//swe)
NATURAL SCIENCES  -- Physical Sciences (hsv//eng)

Keyword

circumstellar matter
supernovae: general
supernovae: individual: LSQ13ddu

Publication and Content Type

ref (subject category)
art (subject category)

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