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• W3098595209 abstract "We study the optical counterpart of the black-hole X-ray binary LMC X-3, by using XMM-Newton/OM observations carried out during a low-hard X-ray state. We derive a better constraint for the temperature, mass and radius of the companion star, and we show that the star is likely to be a ~B5 subgiant filling its Roche lobe. Taking into account the effect of X-ray irradiation, we suggest a value for the mass function in this system, lower than previously thought; we provide a more accurate lower limit to the mass of the compact object." @default.
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• W3098595209 date "2001-01-01" @default.
• W3098595209 modified "2023-09-26" @default.
• W3098595209 title "XMM-Newton optical monitor observations of LMC X-3" @default.
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• W3098595209 doi "https://doi.org/10.1051/0004-6361:20000065" @default.
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