Variability of X-Ray Emission from Cen X-3 Observed with Ginga
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Simplified stellar models like as 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 from nonlinear oscillation of accretion disks or related flow. We studied the variability of Cen X-3 for applying the nonlinear theory to it.
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- Saitou, M., Takeuti, M., and Tanaka, Y.: 1989, Publications of the ASJ 41, 297.Google Scholar