A very massive spectroscopic binary in the LH 54 OB association in the Large Magellanic Cloud

dc.creatorOstrov, Pablo Gabriel
dc.date2002
dc.date2019-11-05T15:11:06Z
dc.identifierhttp://sedici.unlp.edu.ar/handle/10915/84958
dc.identifierissn:0035-8711
dc.descriptionWe announce the discovery of a new early-type, double-lined spectroscopic binary in the LH 54 OB association in the Large Magellanic Cloud. We present a V light curve and radial velocities. We investigate the possible configurations of the system, concluding that it probably contains the most massive star measured at the present, with a mass of the order of 100 M⊙, while its companion has approximately 50 M⊙.
dc.descriptionFacultad de Ciencias Astronómicas y Geofísicas
dc.formatapplication/pdf
dc.format309-314
dc.languageen
dc.rightshttp://creativecommons.org/licenses/by-nc-sa/4.0/
dc.rightsCreative Commons Attribution-NonCommercial-ShareAlike 4.0 International (CC BY-NC-SA 4.0)
dc.subjectCiencias Astronómicas
dc.subjectBinaries: eclipsing
dc.subjectMagellanic clouds
dc.subjectStars: early-type
dc.subjectStars: fundamental parameters
dc.subjectStars: individual: LH 54-425
dc.titleA very massive spectroscopic binary in the LH 54 OB association in the Large Magellanic Cloud
dc.typeArticulo
dc.typeArticulo


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