EXOSAT observations of 4U 1705-44.
Abstract
During a 7-hour observation of 4U 1705-44, the authors detected 6 intensity dips, which show a quasi-periodicity of 1.3 hours. In additon, there are intensity fluctuations in the range of 100 - 500 seconds. These timescales may be interpreted in terms of an orbital period and oscillations of an accretion disc, respectively.
- Publication:
-
X-ray Astronomy 1984
- Pub Date:
- 1985
- Bibcode:
- 1985xra..conf..121L
- Keywords:
-
- Accretion Disks:X-Ray Binaries;
- X-Ray Binaries:Accretion Disks