Hostname: page-component-76c49bb84f-7l7zb Total loading time: 0 Render date: 2025-07-05T10:02:15.319Z Has data issue: false hasContentIssue false
  • English
  • Français

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

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

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.

Information

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