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Close, bright, and boxy : the superluminous SN 2018hti

Fiore, A. (author)
Benetti, S. (author)
Nicholl, M. (author)
show more...
Reguitti, A. (author)
Cappellaro, E. (author)
Campana, S. (author)
Bose, S. (author)
Paraskeva, E. (author)
Berger, E. (author)
Bravo, T. M. (author)
Burke, J. (author)
Cai, Y.-Z. (author)
Chen, Ting-Wan (author)
Stockholms universitet,Institutionen för astronomi,Oskar Klein-centrum för kosmopartikelfysik (OKC)
Chen, P. (author)
Ciolfi, R. (author)
Dong, S. (author)
Gomez, S. (author)
Gromadzki, M. (author)
Gutiérrez, C. P. (author)
Hiramatsu, D. (author)
Hosseinzadeh, G. (author)
Howell, D. A. (author)
Jerkstrand, Anders, 1978- (author)
Stockholms universitet,Institutionen för astronomi,Oskar Klein-centrum för kosmopartikelfysik (OKC)
Kankare, E. (author)
Kozyreva, A. (author)
Maguire, K. (author)
McCully, C. (author)
Ochner, P. (author)
Pellegrino, C. (author)
Pignata, G. (author)
Post, R. S. (author)
Elias-Rosa, N. (author)
Shahbandeh, M. (author)
Schuldt, S. (author)
Thomas, B. P. (author)
Tomasella, L. (author)
Vinkó, J. (author)
Vogl, C. (author)
Wheeler, J. C. (author)
Young, D. R. (author)
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 (creator_code:org_t)
2022-03-17
2022
English.
In: Monthly notices of the Royal Astronomical Society. - : Oxford University Press (OUP). - 0035-8711 .- 1365-2966. ; 512:3, s. 4484-4502
  • Journal article (peer-reviewed)
Abstract Subject headings
Close  
  • SN 2018hti was a very nearby (z = 0.0614) superluminous supernova with an exceedingly bright absolute magnitude of −21.7 mag in r band at maximum. The densely sampled pre-maximum light curves of SN 2018hti show a slow luminosity evolution and constrain the rise time to ∼50 rest-frame d. We fitted synthetic light curves to the photometry to infer the physical parameters of the explosion of SN 2018hti for both the magnetar and the CSM-interaction scenarios. We conclude that one of two mechanisms could be powering the luminosity of SN 2018hti; interaction with ∼10 M⊙ of circumstellar material or a magnetar with a magnetic field of Bp∼ 1.3 × 1013 G, and initial period of Pspin∼ 1.8 ms. From the nebular spectrum modelling we infer that SN 2018hti likely results from the explosion of a ∼40M⊙∼40M⊙ progenitor star.

Subject headings

NATURVETENSKAP  -- Fysik -- Astronomi, astrofysik och kosmologi (hsv//swe)
NATURAL SCIENCES  -- Physical Sciences -- Astronomy, Astrophysics and Cosmology (hsv//eng)

Keyword

supernovae: general
supernovae: individual: SN 2018hti

Publication and Content Type

ref (subject category)
art (subject category)

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