| Issue |
A&A
Volume 407, Number 2, August IV 2003
|
|
|---|---|---|
| Page(s) | 685 - 690 | |
| Section | Stellar structure and evolution | |
| DOI | https://doi.org/10.1051/0004-6361:20030962 | |
| Published online | 17 November 2003 | |
The radial velocity curve of HD 153919 (4U 1700-37) revisited*
1
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
Corresponding author: G. Hammerschlag-Hensberge, godeliev@science.uva.nl
Received:
25
March
2003
Accepted:
17
June
2003
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
([CITE]) and by
Stickland & Lloyd ([CITE]).
Key words: stars: binaries: close / stars: early type / stars: radial velocities / stars: individual: HD 153919 / 4U 1700-37 / ultraviolet: stars
© ESO, 2003
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