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2002MNRAS.336..309O - Mon. Not. R. Astron. Soc., 336, 309-314 (2002/October-2)
A very massive spectroscopic binary in the LH 54 OB association in the Large Magellanic Cloud.
OSTROV P.G.
Abstract (from CDS):
We 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☉.
Abstract Copyright: RAS
Journal keyword(s): binaries: eclipsing - stars: early-type - stars: fundamental parameters - stars: individual: LH 54-425 - Magellanic Clouds.
Simbad objects: 4
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