On The Multiplicity of the Zero-Age Main-Sequence O Star Herschel 36

dc.date.accessioned2020-03-11T20:35:38Z
dc.date.accessioned2022-10-18T23:01:30Z
dc.date.available2020-03-11T20:35:38Z
dc.date.available2022-10-18T23:01:30Z
dc.date.created2020-03-11T20:35:38Z
dc.date.issued2010
dc.identifierhttp://hdl.handle.net/10533/240704
dc.identifier15010003
dc.identifierWOS:000274438700007
dc.identifierno scielo
dc.identifiereid=2-s2.0-77949497400
dc.identifier.urihttps://repositorioslatinoamericanos.uchile.cl/handle/2250/4472043
dc.description.abstractWe present the analysis of high-resolution optical spectroscopic observations of the zero-age main-sequence O star Herschel 36 spanning six years. This star is definitely a multiple system, with at least three components detected in its spectrum. Based on
dc.languageeng
dc.relationhttps://doi.org/10.1088/2041-8205/710/1/L30
dc.relation10.1088/2041-8205/710/1/L30
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.titleOn The Multiplicity of the Zero-Age Main-Sequence O Star Herschel 36
dc.typeArticulo


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