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Photometric and spectroscopic evolution of the interacting transient AT 2016jbu(Gaia16cfr)
cris.lastimport.scopus | 2024-02-12T19:59:35Z |
dc.abstract.en | We present the results from a high-cadence, multiwavelength observation campaign of AT 2016jbu (aka Gaia16cfr), an interacting transient. This data set complements the current literature by adding higher cadence as well as extended coverage of the light-curve evolution and late-time spectroscopic evolution. Photometric coverage reveals that AT 2016jbu underwent significant photometric variability followed by two luminous events, the latter of which reached an absolute magnitude of M<SUB>V</SUB> ~ -18.5 mag. This is similar to the transient SN 2009ip whose nature is still debated. Spectra are dominated by narrow emission lines and show a blue continuum during the peak of the second event. AT 2016jbu shows signatures of a complex, non-homogeneous circumstellar material (CSM). We see slowly evolving asymmetric hydrogen line profiles, with velocities of 500 km s<SUP>-1</SUP> seen in narrow emission features from a slow-moving CSM, and up to 10 000 km s<SUP>-1</SUP> seen in broad absorption from some high-velocity material. Late-time spectra (~+1 yr) show a lack of forbidden emission lines expected from a core-collapse supernova and are dominated by strong emission from H, He I, and Ca II. Strong asymmetric emission features, a bumpy light curve, and continually evolving spectra suggest an inhibit nebular phase. We compare the evolution of H α among SN 2009ip-like transients and find possible evidence for orientation angle effects. The light-curve evolution of AT 2016jbu suggests similar, but not identical, circumstellar environments to other SN 2009ip-like transients. |
dc.affiliation | Uniwersytet Warszawski |
dc.contributor.author | Kankare, E. |
dc.contributor.author | Young, D. R. |
dc.contributor.author | Elias-Rosa, N. |
dc.contributor.author | Skowron, Jan |
dc.contributor.author | Kuncarayakti, H. |
dc.contributor.author | Delgado, A. |
dc.contributor.author | Inserra, C. |
dc.contributor.author | Prieto, J. L. |
dc.contributor.author | Shappee, B. J. |
dc.contributor.author | Meintjes, P. |
dc.contributor.author | Kotak, R. |
dc.contributor.author | Blondin, S. |
dc.contributor.author | Müller-Bravo, T. E. |
dc.contributor.author | Maguire, K. |
dc.contributor.author | Morrell, N. |
dc.contributor.author | Soelen, B. van |
dc.contributor.author | Hanlon, L. |
dc.contributor.author | Dennefeld, M. |
dc.contributor.author | Duffy, P. |
dc.contributor.author | Nyholm, A. |
dc.contributor.author | McCully, C. |
dc.contributor.author | O'Neill, D. |
dc.contributor.author | Callis, E. |
dc.contributor.author | Holoien, T. W. -S. |
dc.contributor.author | Stevance, H. F. |
dc.contributor.author | Dong, Subo |
dc.contributor.author | Nicholl, M. |
dc.contributor.author | Reichart, D. E. |
dc.contributor.author | Leeuwen, M. van |
dc.contributor.author | Martin-Carrillo, A. |
dc.contributor.author | Tucker, B. E. |
dc.contributor.author | Hiramatsu, D. |
dc.contributor.author | Pignata, G. |
dc.contributor.author | Galbany, L. |
dc.contributor.author | Bento, J. |
dc.contributor.author | Cartier, R. |
dc.contributor.author | Benetti, S. |
dc.contributor.author | Sand, D. |
dc.contributor.author | Gromadzki, Mariusz |
dc.contributor.author | Eldridge, J. J. |
dc.contributor.author | Schweyer, T. |
dc.contributor.author | Abbot, H. |
dc.contributor.author | Tartaglia, L. |
dc.contributor.author | Wyrzykowski, Łukasz |
dc.contributor.author | Rau, A. |
dc.contributor.author | Poleski, Radosław |
dc.contributor.author | Szymański, Michał |
dc.contributor.author | Pietrukowicz, Paweł |
dc.contributor.author | Ulaczyk, Krzysztof |
dc.contributor.author | Kozłowski, Szymon |
dc.contributor.author | Pastorello, A. |
dc.contributor.author | Shahbandeh, M. |
dc.contributor.author | Harrison, D. L. |
dc.contributor.author | Hodgkin, S. T. |
dc.contributor.author | Gutiérrez, C. P. |
dc.contributor.author | Hsiao, E. |
dc.contributor.author | Bose, S. |
dc.contributor.author | Chen, Ping |
dc.contributor.author | Smartt, S. J. |
dc.contributor.author | Howell, D. A. |
dc.contributor.author | Sollerman, J. |
dc.contributor.author | Stritzinger, M. D. |
dc.contributor.author | Hosseinzadeh, G. |
dc.contributor.author | Chen, T. -W. |
dc.contributor.author | Brennan, S. J. |
dc.contributor.author | Udalski, Andrzej |
dc.contributor.author | Fraser, M. |
dc.contributor.author | Johansson, J. |
dc.contributor.author | Brown, P. J. |
dc.contributor.author | Soszyński, Igor |
dc.contributor.author | Monard, B. |
dc.date.accessioned | 2024-01-25T16:36:46Z |
dc.date.available | 2024-01-25T16:36:46Z |
dc.date.copyright | 2021-02-18 |
dc.date.issued | 2022 |
dc.description.accesstime | BEFORE_PUBLICATION |
dc.description.finance | Publikacja bezkosztowa |
dc.description.number | 4 |
dc.description.version | ORIGINAL_AUTHOR |
dc.description.volume | 513 |
dc.identifier.doi | 10.1093/MNRAS/STAC1243 |
dc.identifier.issn | 0035-8711 |
dc.identifier.uri | https://repozytorium.uw.edu.pl//handle/item/115843 |
dc.identifier.weblink | http://adsabs.harvard.edu/abs/2022MNRAS.513.5642B |
dc.language | eng |
dc.pbn.affiliation | astronomy |
dc.relation.ispartof | Monthly Notices of the Royal Astronomical Society |
dc.relation.pages | 5642-5665 |
dc.rights | Other |
dc.sciencecloud | nosend |
dc.title | Photometric and spectroscopic evolution of the interacting transient AT 2016jbu(Gaia16cfr) |
dc.type | JournalArticle |
dspace.entity.type | Publication |