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dc.creatorChene, A. N.
dc.date.accessioned2020-03-11T20:36:35Z
dc.date.available2020-03-11T20:36:35Z
dc.date.issued2011
dc.identifier.urihttp://hdl.handle.net/10533/241037
dc.description.abstractAims. What is the origin of the large-amplitude variability in Wolf-Rayet WN8 stars in general and WR123 in particular? A dedicated spectroscopic campaign targets the ten-hour period previously found in the high-precision photometric data obtained by the
dc.language.isoeng
dc.relation.urihttps://doi.org/10.1051/0004-6361/201116567
dc.rightsAtribución-NoComercial-SinDerivadas 3.0 Chile
dc.rightshttp://creativecommons.org/licenses/by-nc-nd/3.0/cl/
dc.titleA 10-h period revealed in optical spectra of the highly variable WN8 Wolf-Rayet star WR 123
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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