Context. Recently, wavelets and R/S analysis have been used as statistical tools to characterize the optical flickering of cataclysmic variables. Aims. Here we present the first comprehensive study of the statistical properties of X-ray flickering of cataclysmic variables in order to link them with physical parameters. Methods. We analyzed a sample of 97 X-ray light curves of 75 objects of all classes observed with the XMM-Newton space telescope. By using the wavelets analysis, each light curve has been characterized by two parameters, alpha and Sigma, that describe the energy distribution of flickering on different timescales and the strength at a given timescale, respectively. We also used the R/S analysis to determine the Hurst exponent of each light curve and define their degree of stochastic memory in time. Results. The X-ray flickering is typically composed of long time scale events (1.5 less than or similar to alpha less than or similar to 3), with very similar strengths in all the subtypes of cataclysmic variables (-3 less than or similar to Sigma less than or similar to -1.5). The X-ray data are distributed in a much smaller area of the alpha-Sigma parameter space with respect to those obtained with optical light curves. The tendency of the optical flickering in magnetic systems to show higher S values than the non-magnetic systems is not encountered in the X-rays. The Hurst exponents estimated for all light curves of the sample are larger than those found in the visible, with a peak at 0.82. In particular, we do not obtain values lower than 0.5. The X-ray flickering presents a persistent memory in time, which seems to be stronger in objects containing magnetic white dwarf primaries. Conclusions. The similarity of the X-ray flickering in objects of different classes together with the predominance of a persistent stochastic behavior can be explained in terms of magnetically-driven accretion processes acting in a considerable fraction of the analyzed objects.
机构:
Ist Nazl Astrofis, Osservatorio Astron Capodimonte, Salita Moiariello 16, I-80131 Naples, Italy
Ist Nazl Astrofis, Osservatorio Astron Roma, Via Frascati 33, I-00040 Monte Porzio Catone, RM, Italy
New York Univ Abu Dhabi, Abu Dhabi 129188, U Arab EmiratesIst Nazl Astrofis, Osservatorio Astron Capodimonte, Salita Moiariello 16, I-80131 Naples, Italy
机构:
Nagoya Univ, Div Particle & Astrophys Sci, Chikusa Ku, Furo Cho, Nagoya, Aichi 4648602, Japan
NASA, Goddard Space Flight Ctr, Code 662, Greenbelt, MD 20771 USANagoya Univ, Div Particle & Astrophys Sci, Chikusa Ku, Furo Cho, Nagoya, Aichi 4648602, Japan
Hayashi, Takayuki
Kitaguchi, Takao
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Hiroshima Univ, Dept Phys Sci, 1-3-1 Kagamiyama, Higashihiroshima, Hiroshima 7398526, Japan
Hiroshima Univ, Core Res Energet Universe, 1-3-1 Kagamiyama, Higashihiroshima, Hiroshima 7398526, JapanNagoya Univ, Div Particle & Astrophys Sci, Chikusa Ku, Furo Cho, Nagoya, Aichi 4648602, Japan
Kitaguchi, Takao
Ishida, Manabu
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Inst Space & Astronaut Sci JAXA, Chuo Ku, 3-1-1 Yoshinodai, Sagamihara, Kanagawa 2525210, Japan
Tokyo Metropolitan Univ, Dept Phys, 1-1 Minami Osawa, Hachioji, Tokyo 1920397, JapanNagoya Univ, Div Particle & Astrophys Sci, Chikusa Ku, Furo Cho, Nagoya, Aichi 4648602, Japan