VLTI/MIDI observations of the circumstellar shell of an AGB star: W Hydrae

dc.date.accessioned2020-08-04T21:50:44Z
dc.date.accessioned2022-10-18T23:14:40Z
dc.date.available2020-08-04T21:50:44Z
dc.date.available2022-10-18T23:14:40Z
dc.date.created2020-08-04T21:50:44Z
dc.date.issued2003
dc.identifierhttp://hdl.handle.net/10533/242473
dc.identifier15010003
dc.identifier.urihttps://repositorioslatinoamericanos.uchile.cl/handle/2250/4473763
dc.description.abstractW Hydrae is a prototype AGB star with a dusty circumstellar shell. The shell is marginally resolved at ground-based subarcsecond resolution; the unresolved dust condensation radius is expected to be of order 30 50 mas. Since the dusty circumstellar shell
dc.languageeng
dc.publisherPerrin, G.
dc.publisherMalbet, F.
dc.publisherLes Houches
dc.relationhttp://www.jmmc.fr/mirrors/obsvlti/book/DeGrijs.pdf
dc.relationinstname: ANID
dc.relationreponame: Repositorio Digital RI2.0
dc.rightsinfo:eu-repo/semantics/openAccess
dc.rightsAtribución-NoComercial-SinDerivadas 3.0 Chile
dc.rightshttp://creativecommons.org/licenses/by-nc-nd/3.0/cl/
dc.titleVLTI/MIDI observations of the circumstellar shell of an AGB star: W Hydrae
dc.typeCapitulo de libro


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