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X-Ray Fluctuations from the Advection-Dominated Accretion Disk with a Critical Behavior

Published online by Cambridge University Press:  25 May 2016

M. Takeuchi
M. Takeuchi*
Affiliation:
Kyoto University, Department of Astronomy Sakyo-ku, Kyoto, 606-01, JAPAN

Extract

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The new model for X-ray fluctuations of Cyg X-1, which is based on the fluid dynamics, is presented. The model is the optically thin and advection-dominated accretion disk model, which has a critical behavior.

Type
Session 3: Diagnostics of High Gravity Objects with X- and Gamma Rays
Information
Symposium - International Astronomical Union , Volume 188: The Hot Universe , 1998 , pp. 404 - 405
Copyright
Copyright © Kluwer 1998 

References

Takeuchi, M., & Mineshige, S. (1997) X-ray Fluctuations from the Advection-Dominated Accretion Disks with A critical Behavior ApJ , 486, 160–168 Google Scholar