Physics
Scientific paper
Dec 1993
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993adspr..13r.291b&link_type=abstract
Advances in Space Research, Vol. 13, No. 12, p. 291 - 294
Physics
Scientific paper
The authors have simulated, using a Monte Carlo method, intensity time series representing the time behaviour of some high mass X ray binaries. Taking into account some physical models of the accretion processes, they have parametrized different physical conditions on the source. The resulting time series have been analysed by Fast Fourier Transform techniques. Using different sets of parameters one has been able to generate power spectra of different shapes. Some preliminary results of these simulations and a comparison with an observed spectrum of a galactic X ray binary are discussed.
Burderi Luciano
Cusumano Giancarlo
Robba Natale Renato
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