YITP WORKSHOP ON
Quasi-Periodic Oscillations and Time Variabilities of Accretion Flows
 
ABSTRACT

NAME
INSTITUTE
TITLE OF THE TALK
G. Torok
Silesian Univ., Czech Republic
Orbital models of high frequency QPOs
It is most often supposed that high frequency QPOs originate in an orbital motion near the inner edge of an accretion disk. We discuss recently noticed strong restrictions to orbital QPO models following from the analysis of QPO amplitude behaviour in a group of sources.


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