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dc.creatorTylenda, R.
dc.creatorPietrzynski, G.
dc.date.accessioned2020-03-11T20:36:29Z
dc.date.available2020-03-11T20:36:29Z
dc.date.issued2011
dc.identifier.urihttp://hdl.handle.net/10533/240987
dc.description.abstractStellar mergers are expected to take place in numerous circumstences in the evolution of stellar systems. In particular, they are considered as a plausible origin of stellar eruptions of the V838 Mon type. V1309 Sco is the most recent eruption of this typ
dc.language.isoeng
dc.relation.urihttps://doi.org/10.1051/0004-6361/201016221
dc.rightsAtribución-NoComercial-SinDerivadas 3.0 Chile
dc.rightshttp://creativecommons.org/licenses/by-nc-nd/3.0/cl/
dc.titleV1309 Scorpii: merger of a contact binary
dc.typeArticulo
dc.identifier.folio15010003
dc.description.conicytprogramFONDAP
dc.rights.driverinfo:eu-repo/semantics/openAccess
dc.title.journalAstronomy & Astrophysics
dc.type.driverinfo:eu-repo/semantics/article
dc.description.shortconicytprogramFONDAP
dc.type.openaireinfo:eu-repo/semantics/publishedVersion


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