Journal
ASTRONOMY & ASTROPHYSICS
Volume 365, Issue 1, Pages L273-L276Publisher
EDP SCIENCES S A
DOI: 10.1051/0004-6361:20000065
Keywords
accretion, accretion disks; black hole physics; binaries : general; stars : early type; X-rays : general
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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 similar to B5 subgiant filling its Roche lobe. Taking into account the Effect of X-ray irradiation, we suggest a value f(M) approximate to 1.5 M. 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.
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