Optical spectroscopy of the X-ray transient XTE J1118+480 in outburst

We report on optical spectroscopic observations of the X-ray transient XTE J1118+480 covering the period from 2000 April 7 to July 4. The spectrum is characterized by weak, broad, double-peaked Balmer and He lines on top of a blue continuum of slope p approximate to 1/3, as expected for an optically thick accretion disk. The weak Bowen blend seen in our spectra may indicat e a low metallicity for the source. The presence of a partial S-wave patter n in the He II lambda 4686 line appears consistent with the reported photom etric period P-orb = 4.1 hr for XTE J1118+480. By using a combination of Do ppler mapping and various theoretical arguments, we constrain plausible orb ital parameters for the system: a mass ratio 0.02 less than or similar to q less than or similar to 0.1 and an inclination i less than or similar to 7 0 degrees for a neutron star primary or 30 degrees less than or similar to i less than or similar to 50 degrees for a black hole primary with a mass b etween 4 and 10 M-circle dot. Ca II absorption features observed at very hi gh resolution constrain the interstellar hydrogen absorption column log [N- HI(cm(-2))] approximate to 20.45 + 0.2, and the identification of three abs orbing clouds indicate a distance to the source less than or similar to1 kp c, assuming the line of sight to XTE J1118+480 has average high-latitude pr operties. These results are discussed in the context of previous multiwavel ength observations of this unusual system.