Bibcode
Barnes, A. D.; Casares, J.; Cornelisse, R.; Charles, P. A.; Steeghs, D.; Hynes, R. I.; O'Brien, K.
Bibliographical reference
Monthly Notices of the Royal Astronomical Society, Volume 380, Issue 3, pp. 1182-1190.
Advertised on:
9
2007
Citations
17
Refereed citations
13
Description
We present simultaneous high-resolution optical spectroscopy and X-ray
data of the X-ray binary system GRMus (XB1254-690), obtained over a full
range of orbital phases. The X-ray observations are used to re-establish
the orbital ephemeris for this source. The optical data include the
first spectroscopic detection of the donor star in this system through
the use of the Doppler Tomography technique on the Bowen fluorescence
blend (~4630-4650 Å). In combination with an estimate for the
orbital parameters of the compact object using the wings of the HeII
λ4686 emission line, dynamical mass constraints of 1.20 <=
MX/Msolar <= 2.64 for the neutron star and 0.45
<= M2/Msolar <= 0.85 for the companion are
derived.