SIMBAD references

New high-quality light curves of the late-type binary system BH Vir have been obtained during a 6 year photometric uvby and Hβ monitoring program of low mass eclipsing binaries (Clement et al., 1997A&AS..123....1C and 1997A&AS..123...59C), hereafter Papers I and II. This paper presents detailed analysis of this binary based on the four light curves obtained within our program. The activity wave superimposed on the eclipse-modulated light curves has been adjusted and removed by using a new iterative application of the standard EBOP code together with truncated Fourier Series fittings. Combining the recent radial velocity curves (Popper, 1995) with the geometrical elements deduced from the ``clean" photometric light curves, the absolute parameters of the system are calculated. BH Vir appears as a binary composed by two main sequence G0 and G2 stars with solar chemical composition lying on the same isochrone (log(τ)=9.8±0.2years). The accuracy obtained on the absolute parameters determination allows us to include BH Vir on the select group of late-type stars to be used on the estimation of the Mass-Luminosity-Relationship.