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Simulation of Aperiodic and Periodic Variabilities in X-RAY Sources
L. Burderi, M. Guainazzi, N. R. Robba
Istituto di Fisica, Universitá di Palermo, Via Archirafi 36, I-
90133 Palermo, Italy
The Power Spectrum
Density (PSD) has been extensively used to study the periodic (Harmonic
Lines, HL) and the aperiodic (Red Noise, RN) features of the temporal
variability of the High Mass X Ray Binaries (HMXRB). Some authors have
proposed a very simple Shot Noise model (SN) in order to explain the RN
feature (Terrel and Olsen 1970). In this scenario the plasma instabilities that can occur during
the accretion process (Rayleigh-Taylor, Kelvin-Helmoltz, Alfvén zone
instabilities above the accretion column)
could clump the matter in blobs (Elsner and Lamb 1977,1984;
Arons and Lea 1976); the shot emission
associated with the accretion of these blobs is the cause of the aperiodic
variability. The timescale associated with the instabilities
mentioned above cover a very wide range (roughly from milliseconds to
tens of seconds). Due to the casual
occurrence of the blobs, as a consequence of the instability phenomena,
these emissions are supposed to occur randomly (stochastically) in time.
This article was taken from
http://www.astro.lsa.umich.edu/users/iotm/oct95/orion.html
The rest of the article can be viewed at that site.
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