Astronomy and Astrophysics – Astronomy
Scientific paper
Feb 1992
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992mnras.254..419w&link_type=abstract
Monthly Notices of the Royal Astronomical Society (ISSN 0035-8711), vol. 254, Feb. 1, 1992, p. 419-426. Research supported by Un
Astronomy and Astrophysics
Astronomy
13
Eclipsing Binary Stars, Magellanic Clouds, Stellar Spectrophotometry, Variable Stars, Visual Photometry, B Stars, Charge Coupled Devices, Light Curve, O Stars, Stellar Temperature, Symbiotic Stars
Scientific paper
CCD BVI photometry is presented of the light curves of the eclipsing binary stars HV 2208 in the Small Magellanic Cloud and HV 12634 in the Large Magellanic Cloud. Precisions attained are 1.5-2.0 percent. A preliminary analysis suggests that HV 2208 could comprise components similar to galactic B0.5 V and B4 III stars, with the secondary filling its Roche lobe and having lost mass, but that the OB components of HV 12634 must be hotter for their mass and radius than typical galactic stars.
Gilmore Alan C.
Tobin William
West R. D. S.
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