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Close, bright, and ...
Close, bright, and boxy : the superluminous SN 2018hti
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Fiore, A. (author)
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Benetti, S. (author)
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Nicholl, M. (author)
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show more...
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Reguitti, A. (author)
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Cappellaro, E. (author)
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Campana, S. (author)
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Bose, S. (author)
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Paraskeva, E. (author)
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Berger, E. (author)
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Bravo, T. M. (author)
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Burke, J. (author)
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Cai, Y.-Z. (author)
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- Chen, Ting-Wan (author)
- Stockholms universitet,Institutionen för astronomi,Oskar Klein-centrum för kosmopartikelfysik (OKC)
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Chen, P. (author)
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Ciolfi, R. (author)
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Dong, S. (author)
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Gomez, S. (author)
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Gromadzki, M. (author)
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Gutiérrez, C. P. (author)
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Hiramatsu, D. (author)
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Hosseinzadeh, G. (author)
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Howell, D. A. (author)
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- Jerkstrand, Anders, 1978- (author)
- Stockholms universitet,Institutionen för astronomi,Oskar Klein-centrum för kosmopartikelfysik (OKC)
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Kankare, E. (author)
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Kozyreva, A. (author)
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Maguire, K. (author)
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McCully, C. (author)
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Ochner, P. (author)
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Pellegrino, C. (author)
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Pignata, G. (author)
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Post, R. S. (author)
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Elias-Rosa, N. (author)
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Shahbandeh, M. (author)
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Schuldt, S. (author)
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Thomas, B. P. (author)
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Tomasella, L. (author)
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Vinkó, J. (author)
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Vogl, C. (author)
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Wheeler, J. C. (author)
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Young, D. R. (author)
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(creator_code:org_t)
- 2022-03-17
- 2022
- English.
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In: Monthly notices of the Royal Astronomical Society. - : Oxford University Press (OUP). - 0035-8711 .- 1365-2966. ; 512:3, s. 4484-4502
- Related links:
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https://urn.kb.se/re...
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https://doi.org/10.1...
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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)
Find in a library
To the university's database
- By the author/editor
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Fiore, A.
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Benetti, S.
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Nicholl, M.
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Reguitti, A.
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Cappellaro, E.
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Campana, S.
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show more...
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Bose, S.
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Paraskeva, E.
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Berger, E.
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Bravo, T. M.
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Burke, J.
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Cai, Y.-Z.
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Chen, Ting-Wan
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Chen, P.
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Ciolfi, R.
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Dong, S.
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Gomez, S.
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Gromadzki, M.
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Gutiérrez, C. P.
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Hiramatsu, D.
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Hosseinzadeh, G.
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Howell, D. A.
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Jerkstrand, Ande ...
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Kankare, E.
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Kozyreva, A.
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Maguire, K.
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McCully, C.
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Ochner, P.
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Pellegrino, C.
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Pignata, G.
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Post, R. S.
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Elias-Rosa, N.
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Shahbandeh, M.
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Schuldt, S.
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Thomas, B. P.
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Tomasella, L.
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Vinkó, J.
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Vogl, C.
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Wheeler, J. C.
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Young, D. R.
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show less...
- About the subject
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- NATURAL SCIENCES
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NATURAL SCIENCES
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and Physical Science ...
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and Astronomy Astrop ...
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Monthly notices ...
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Stockholm University