Astrophysical Journal

dc.creatorRest, A.
dc.creatorClocchiatti, A.
dc.creatorMinniti, D.
dc.creatorPrieto, J. L.
dc.creatorPietrzynski, G.
dc.date2020-03-11T20:36:37Z
dc.date2022-07-08T17:16:49Z
dc.date2020-03-11T20:36:37Z
dc.date2022-07-08T17:16:49Z
dc.date2011
dc.date.accessioned2023-08-23T00:34:25Z
dc.date.available2023-08-23T00:34:25Z
dc.identifier15010003
dc.identifier15010003
dc.identifierhttps://hdl.handle.net/10533/241050
dc.identifier.urihttps://repositorioslatinoamericanos.uchile.cl/handle/2250/8355641
dc.descriptionWe report the discovery of a supernova (SN) with the highest apparent energy output to date and conclude that it represents an extreme example of the Type IIn subclass. The SN, which was discovered behind the Large Magellanic Cloud at z = 0.289 by the Sup
dc.descriptionFONDAP
dc.descriptionFONDAP
dc.languageeng
dc.relationhttps://doi.org/10.1088/0004-637X/729/2/88
dc.rightsAtribución-NoComercial-SinDerivadas 3.0 Chile
dc.rightshttp://creativecommons.org/licenses/by-nc-nd/3.0/cl/
dc.rightsinfo:eu-repo/semantics/openAccess
dc.titlePushing the Boundaries of Conventional Core-collapse Supernovae: The Extremely Energetic Supernova SN 2003ma
dc.titleAstrophysical Journal
dc.typeArticulo
dc.typeinfo:eu-repo/semantics/article
dc.typeinfo:eu-repo/semantics/publishedVersion


Este ítem pertenece a la siguiente institución