Phase lags of quasi-periodic oscillations across source states in the low-mass X-ray binary 4U 1636_53

5th Compact Stars in the QCD Phase Diagram

De Avellar, Marcio G.B.^1

Instituto de Astronomia, Geofísica e de Ciências Atmosféricas, Universidade de São Paulo, Rua do Matão 1226, Sãao Paulo

05508-090, Brazil^1

关键词: Comptonization;    Dynamical model;    Extreme environment;    Light curves;    Low-mass X-ray binaries;    Physical conditions;    Quasiperiodic oscillations;    Radiative process;   

Others  :  https://iopscience.iop.org/article/10.1088/1742-6596/861/1/012004/pdf
DOI  :  10.1088/1742-6596/861/1/012004

来源: IOP

【 摘 要 】

The majority of attempts to explain the origin and phenomenology of the quasi-periodic oscillations (QPOs) detected in low-mass X-ray binaries invoke dynamical models, and it was just in recent years that renewed attention has been given on how radiative processes occurring in these extreme environments gives rise to the variability features observed in the X-ray light curves of these systems. The study of the dependence of the phase lags upon the energy and frequency of the QPOs is a step towards this end. The methodology we developed here allowed us to study for the first time these dependencies for all QPOs detected in the range of 1 to 1300 Hz in the low-mass X-ray binary 4U 1636-53 as the source changes its state during its cycle in the colour-colour diagram. Our results suggest that within the context of models of up-scattering Comptonization, the phase lags dependencies upon frequency and energy can be used to extract size scales and physical conditions of the medium that produces the lags.