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SN 2017ens: The Metamorphosis of a Luminous Broadlined Type Ic Supernova into an SN IIn
cris.lastimport.scopus | 2024-02-12T20:56:58Z |
dc.abstract.en | We present observations of supernova (SN) 2017ens, discovered by the ATLAS survey and identified as a hot blue object through the GREAT program. The redshift z = 0.1086 implies a peak brightness of M <SUB> g </SUB> = -21.1 mag, placing the object within the regime of superluminous supernovae. We observe a dramatic spectral evolution, from initially being blue and featureless, to later developing features similar to those of the broadlined Type Ic SN 1998bw, and finally showing Ė2000 km s<SUP>-1</SUP> wide HĪ± and HĪ² emission. Relatively narrow Balmer emission (reminiscent of a SN IIn) is present at all times. We also detect coronal lines, indicative of a dense circumstellar medium. We constrain the progenitor wind velocity to Ė50-60 km s<SUP>-1</SUP> based on P-Cygni profiles, which is far slower than those present in Wolf-Rayet stars. This may suggest that the progenitor passed through a luminous blue variable phase, or that the wind is instead from a binary companion red supergiant star. At late times we see the Ė2000 km s<SUP>-1</SUP> wide HĪ± emission persisting at high luminosity (Ė3 Ć 10<SUP>40</SUP> erg s<SUP>-1</SUP>) for at least 100 day, perhaps indicative of additional mass loss at high velocities that could have been ejected by a pulsational pair instability. |
dc.affiliation | Uniwersytet Warszawski |
dc.contributor.author | Chen, T. -W. |
dc.contributor.author | Inserra, C. |
dc.contributor.author | Fraser, M. |
dc.contributor.author | Moriya, T. J. |
dc.contributor.author | Schady, P. |
dc.contributor.author | Schweyer, T. |
dc.contributor.author | Filippenko, A. V. |
dc.contributor.author | Perley, D. A. |
dc.contributor.author | Ruiter, A. J. |
dc.contributor.author | Seitenzahl, I. |
dc.contributor.author | Sollerman, J. |
dc.contributor.author | Taddia, F. |
dc.contributor.author | Anderson, J. P. |
dc.contributor.author | Foley, R. J. |
dc.contributor.author | Jerkstrand, A. |
dc.contributor.author | Ngeow, C. -C. |
dc.contributor.author | Pan, Y. -C. |
dc.contributor.author | Pastorello, A. |
dc.contributor.author | Points, S. |
dc.contributor.author | Smartt, S. J. |
dc.contributor.author | Smith, K. W. |
dc.contributor.author | Taubenberger, S. |
dc.contributor.author | Wiseman, P. |
dc.contributor.author | Young, D. R. |
dc.contributor.author | Benetti, S. |
dc.contributor.author | Berton, M. |
dc.contributor.author | Bufano, F. |
dc.contributor.author | Clark, P. |
dc.contributor.author | Valle, M. Della |
dc.contributor.author | Galbany, L. |
dc.contributor.author | Gal-Yam, A. |
dc.contributor.author | Gromadzki, Mariusz |
dc.contributor.author | GutiƩrrez, C. P. |
dc.contributor.author | Heinze, A. |
dc.contributor.author | Kankare, E. |
dc.contributor.author | Kilpatrick, C. D. |
dc.contributor.author | Kuncarayakti, H. |
dc.contributor.author | Leloudas, G. |
dc.contributor.author | Lin, Z. -Y. |
dc.contributor.author | Maguire, K. |
dc.contributor.author | Mazzali, P. |
dc.contributor.author | McBrien, O. |
dc.contributor.author | Prentice, S. J. |
dc.contributor.author | Rau, A. |
dc.contributor.author | Rest, A. |
dc.contributor.author | Siebert, M. R. |
dc.contributor.author | Stalder, B. |
dc.contributor.author | Tonry, J. L. |
dc.contributor.author | Yu, P. -C. |
dc.date.accessioned | 2024-01-26T07:50:07Z |
dc.date.available | 2024-01-26T07:50:07Z |
dc.date.copyright | 2018-08-13 |
dc.date.issued | 2018 |
dc.description.accesstime | BEFORE_PUBLICATION |
dc.description.finance | Nie dotyczy |
dc.description.number | 2 |
dc.description.version | ORIGINAL_AUTHOR |
dc.description.volume | 867 |
dc.identifier.doi | 10.3847/2041-8213/AAEB2E |
dc.identifier.issn | 2041-8205 |
dc.identifier.uri | https://repozytorium.uw.edu.pl//handle/item/120060 |
dc.identifier.weblink | http://adsabs.harvard.edu/abs/2018ApJ...867L..31C |
dc.language | eng |
dc.pbn.affiliation | astronomy |
dc.relation.ispartof | Astrophysical Journal Letters |
dc.relation.pages | L31 |
dc.rights | Other |
dc.sciencecloud | nosend |
dc.title | SN 2017ens: The Metamorphosis of a Luminous Broadlined Type Ic Supernova into an SN IIn |
dc.type | JournalArticle |
dspace.entity.type | Publication |