Astronomy: ASASSN-15lh: A highly super-luminous supernova
dc.contributor.author | Dong, Subo | |
dc.contributor.author | Shappee, B.J. | |
dc.contributor.author | Prieto, J.L. | |
dc.contributor.author | Jha, S.W. | |
dc.contributor.author | Stanek, K.Z. | |
dc.contributor.author | Holoien, T.W.-S. | |
dc.contributor.author | Kochanek, C.S. | |
dc.contributor.author | Thompson, T.A. | |
dc.contributor.author | Morrell, N. | |
dc.contributor.author | Thompson, I.B. | |
dc.contributor.author | Basu, U. | |
dc.contributor.author | Beacom, J.F. | |
dc.contributor.author | Bersier, D. | |
dc.contributor.author | Brimacombe, J. | |
dc.contributor.author | Brown, J.S. | |
dc.contributor.author | Bufano, F. | |
dc.contributor.author | Chen, Ping | |
dc.contributor.author | Conseil, E. | |
dc.contributor.author | Danilet, A.B. | |
dc.contributor.author | Falco, E. | |
dc.contributor.author | Grupe, D. | |
dc.contributor.author | Kiyota, S. | |
dc.contributor.author | Masi, G. | |
dc.contributor.author | Nicholls, B. | |
dc.contributor.author | Olivares, F.E. | |
dc.contributor.author | Pignata, G. | |
dc.contributor.author | Pojmanski, G. | |
dc.contributor.author | Simonian, G.V. | |
dc.contributor.author | Szczygiel, D.M. | |
dc.contributor.author | Woźniak, P.R. | |
dc.date.accessioned | 2023-11-22T14:57:18Z | |
dc.date.available | 2023-11-22T14:57:18Z | |
dc.date.issued | 2016-01 | |
dc.description | Indexación: Scopus. | es |
dc.description.abstract | We report the discovery of ASASSN-15lh (SN 2015L), which we interpret as the most luminous supernova yet found. At redshift z = 0.2326, ASASSN-15lh reached an absolute magnitude of Mu,AB = –23.5 ± 0.1 and bolometric luminosity Lbol = (2.2 ± 0.2) × 1045 ergs s–1, which is more than twice as luminous as any previously known supernova. It has several major features characteristic of the hydrogen-poor super-luminous supernovae (SLSNe-I), whose energy sources and progenitors are currently poorly understood. In contrast to most previously known SLSNe-I that reside in star-forming dwarf galaxies, ASASSN-15lh appears to be hosted by a luminous galaxy (MK ≈ –25.5) with little star formation. In the 4 months since first detection, ASASSN-15lh radiated (1.1 ± 0.2) × 1052 ergs, challenging the magnetar model for its engine. | es |
dc.description.uri | https://www-science-org.recursosbiblioteca.unab.cl/doi/10.1126/science.aac9613 | |
dc.identifier.citation | Science. Volume 351, Issue 6270, Pages 257 - 260. 15 January 2016 | es |
dc.identifier.doi | 10.1126/science.aac9613 | |
dc.identifier.issn | 0036-8075 | |
dc.identifier.uri | https://repositorio.unab.cl/xmlui/handle/ria/54020 | |
dc.language.iso | en | es |
dc.publisher | American Association for the Advancement of Science | es |
dc.subject | ASASSN-15lh (SN 2015L) | es |
dc.subject | Most Luminous Supernova | es |
dc.title | Astronomy: ASASSN-15lh: A highly super-luminous supernova | es |
dc.type | Artículo | es |
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