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Variability of X-Ray Emission from Cen X-3 Observed with Ginga

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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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Copyright information

© Springer Science+Business Media Dordrecht 1993

Authors and Affiliations

  1. 1.Astronomical InstituteTôhoku UniversitySendai 980Japan
  2. 2.Institute of Space and Astronautical ScienceSagamihara 229Japan
  3. 3.Department of PhysicsUniversity of TokyoBunkyo-ku, Tokyo 113Japan

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