Abstract
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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© 1993 Springer Science+Business Media Dordrecht
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Kanetake, R., Takeshima, T., Makishima, K., Takeuti, M. (1993). Variability of X-Ray Emission from Cen X-3 Observed with Ginga. In: Takeuti, M., Buchler, JR. (eds) Nonlinear Phenomena in Stellar Variability. Springer, Dordrecht. https://doi.org/10.1007/978-94-011-1062-4_11
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DOI: https://doi.org/10.1007/978-94-011-1062-4_11
Publisher Name: Springer, Dordrecht
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