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  SN 2020wnt: a slow-evolving carbon-rich superluminous supernova with no O ii lines and a bumpy light curve

Gutiérrez, C. P., Pastorello, A., Bersten, M., Benetti, S., Orellana, M., Fiore, A., et al. (2022). SN 2020wnt: a slow-evolving carbon-rich superluminous supernova with no O ii lines and a bumpy light curve. Monthly Notices of the Royal Astronomical Society, 517(2), 2056-2075. doi:10.1093/mnras/stac2747.

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Gutiérrez, C. P., Author
Pastorello, A., Author
Bersten, M., Author
Benetti, S., Author
Orellana, M., Author
Fiore, A., Author
Karamehmetoglu, E., Author
Kravtsov, T., Author
Reguitti, A., Author
Reynolds, T. M., Author
Valerin, G., Author
Mazzali, P.1, Author           
Sullivan, M., Author
Cai, Y.-Z., Author
Elias-Rosa, N., Author
Fraser, M., Author
Hsiao, E. Y., Author
Kankare, E., Author
Kotak, R., Author
Kuncarayakti, H., Author
Li, Z., AuthorMattila, S., AuthorMo, J., AuthorMoran, S., AuthorOchner, P., AuthorShahbandeh, M., AuthorTomasella, L., AuthorWang, X., AuthorYan, S., AuthorZhang, J., AuthorZhang, T., AuthorStritzinger, M. D., Author more..
Affiliations:
1Stellar Astrophysics, MPI for Astrophysics, Max Planck Society, ou_159882              

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 Dates: 2022-09-26
 Publication Status: Published online
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 Identifiers: DOI: 10.1093/mnras/stac2747
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Title: Monthly Notices of the Royal Astronomical Society
Source Genre: Journal
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Pages: - Volume / Issue: 517 (2) Sequence Number: - Start / End Page: 2056 - 2075 Identifier: -