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A&A 407, 685-690 (2003)
DOI: 10.1051/0004-6361:20030962
The radial velocity curve of HD 153919 (4U 1700-37) revisited
G. Hammerschlag-Hensberge1, M. H. van Kerkwijk2, 3 and L. Kaper11 Astronomical Institute "Anton Pannekoek" and Center for High-Energy Astrophysics, University of Amsterdam, Kruislaan 403, 1098 SJ Amsterdam, The Netherlands
2 Astronomical Institute, Utrecht University, PO Box 80000, 3508 TA Utrecht, The Netherlands
3 Dept. of Astronomy & Astrophysics, 60 St George Street, Toronto, ON, M5S 3H8, Canada
(Received 25 March 2003 / Accepted 17 June 2003 )
Abstract
We have re-analysed all available high-resolution
ultraviolet IUE spectra of the high-mass X-ray binary
HD 153919/4U 1700-37. The radial velocity semi-amplitude of
km s
-1 and orbital eccentricity of
agree very well
with the values obtained earlier from optical spectra. They disagree
with earlier conclusions for the same data reduced by Heap & Corcoran
(1992) and by
Stickland & Lloyd (1993).
Key words: stars: binaries: close -- stars: early type -- stars: radial velocities -- stars: individual: HD 153919 -- 4U 1700-37 -- ultraviolet: stars
Offprint request: G. Hammerschlag-Hensberge, godeliev@science.uva.nl
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© ESO 2003
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