The identification of the long-period X-ray pulsar 1WGA J1958.2+3232 with a Be-star/X-ray binary

We present the results of optical observations performed between May and September 1998 of the stars within the position error circle of the recently discovered ~ 12 min pulsating X-ray source 1WGA J1958.2+3232 . Based on photometry and slitless spectroscopy, we selected a likely optical counterpart, which was subsequently determined to be a m_V=15.7 B0Ve star, the spectral properties of which are in good agreement with the X-ray results. The proposed optical counterpart shows several H, He and Fe emission-lines, while the interstellar absorption spectral features place the star at a distance of ~ 800 pc. The inferred X-ray luminosity for this distance is =~ 10(33) erg s(-1) in the 2-10 keV band. We conclude that 1WGA J1958.2+3232 is a likely new long-period low-luminosity accreting neutron star in a Be-star/X-ray binary system. Based on data collected at the Astronomical Observatory of Loiano, Italy