I. Negueruela et al., OPTICAL AND INFRARED OBSERVATIONS OF THE SUSPECTED BE X-RAY TRANSIENT4U-0728-25/, Astronomy and astrophysics, 315(1), 1996, pp. 160-165
We present new optical spectra and photometry plus the first infrared
photometry of the optical counterpart to the X-ray transient system 4U
0728-25. Our spectral and photometrical analysis lead us to conclude
that the primary is an O8-9Ve star with E(B - V) = 0.75 +/- 0.02. This
revised spectral classification places the star at a distance of 6.1/-0.3 kpc, We also present evidence for an unusual faint, blue state t
hat may represent a diskless phase in late 1991.