Variability of X-Ray Emission from CEN X-3 Observed with GINGA
Abstract
Simplified stellar models like one-zone models can be oscillated in chaotic state (Saitou et al. 1989). It is natural to consider that the irregular variations of Galactic X-ray sources might be caused by nonlinear oscillation of accretion disks or related flow. We studied the variability of Cen X-3 and applied the nonlinear theory to it.
- Publication:
-
Astrophysics and Space Science
- Pub Date:
- December 1993
- DOI:
- 10.1007/BF00657879
- Bibcode:
- 1993Ap&SS.210..113K
- Keywords:
-
- Accretion Disks;
- Chaos;
- Stellar Models;
- Stellar Oscillations;
- X Ray Sources;
- Emission Spectra;
- Ginga Satellite;
- Light Curve;
- Periodic Variations;
- Astrophysics