Comparison of the Hαcircumstellar disks in Be/X-ray binaries and Be stars
Open Access
- 15 March 2001
- journal article
- Published by EDP Sciences in Astronomy & Astrophysics
- Vol. 367 (3) , 884-890
- https://doi.org/10.1051/0004-6361:20000533
Abstract
Astronomy & Astrophysics (A&A) is an international journal which publishes papers on all aspects of astronomy and astrophysicsKeywords
All Related Versions
This publication has 18 references indexed in Scilit:
- The Be/X-ray transient V0332+53: evidence for a tilt between the orbit and the equatorial plane?Monthly Notices of the Royal Astronomical Society, 1999
- Long-term variability of the Be/X-ray binary A 0535+26 -- I. Optical and UV spectroscopyMonthly Notices of the Royal Astronomical Society, 1998
- Fundamental parameters, helium abundance and distance of X PerseiMonthly Notices of the Royal Astronomical Society, 1997
- Equatorial disk formation around rotating stars due to Ram pressure confinement by the stellar windThe Astrophysical Journal, 1993
- Stellarv sini and optical emission line widths in Be starsAstrophysics and Space Science, 1989
- Spectral variability of 4U1145-619 during X-ray outburstMonthly Notices of the Royal Astronomical Society, 1987
- The three types of high-mass X-ray pulsatorMonthly Notices of the Royal Astronomical Society, 1986
- Spectroscopy of the unique degenerate binary star LSI + 61 deg 303Publications of the Astronomical Society of the Pacific, 1981
- The optical counterpart of 4U 0115+63The Astrophysical Journal, 1981
- Profiles of Emission Lines in be StarsThe Astrophysical Journal, 1972