Photometry, Spectroscopy, And Doppler Tomography Of The Eclipsing LMXB EXO 0748-676 = UY Vol

Astronomy and Astrophysics – Astronomy

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We present optical spectra and Doppler tomography of the low-mass X-ray binary EXO 0748-676 = UY Vol. UY Vol is an eclipsing X-ray binary hosting a neutron star. With a total of 65 spectra spread over 4 nights, we have complete phase coverage and construct trailed spectra and Doppler tomograms for thirteen lines and line blends. Although we were not able to detect fluorescent N III/C III emission from the irradiated secondary, we do detect S-wave emission of several He II lines and O II 5289A. Our analysis of the trailed spectra and tomograms allows us to constrain the origin of the line emission. UY Vol has spent the better part of the last two decades in a burst state, but since our spectroscopy, the source has entered a quiescent phase. The optical counterpart, originally 17th mag has faded substantially to R 22 mag. We present a new light-curve of the source in its quiescent state.
This work is partially supported by the National Science Foundation under Grant No. AST-0908789 and by NASA/Louisiana Board of Regents grant NNX07AT62A/LEQSF(2007-10) Phase3-02.

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