Vertical Structure of the Outer Accretion Disk in Persistent Low-Mass X-Ray Binaries
arXiv:1108.4222 · doi:10.1134/S1063773711050045
Abstract
We have investigated the influence of X-ray irradiation on the vertical structure of the outer accretion disk in low-mass X-ray binaries by performing a self-consistent calculation of the vertical structure and X-ray radiation transfer in the disk. Penetrating deep into the disk, the field of scattered X-ray photons with energy \,keV exerts a significant influence on the vertical structure of the accretion disk at a distance \,cm from the neutron star. At a distance \,cm, where the total surface density in the disk reaches \,g\,cm, X-ray heating affects all layers of an optically thick disk. The X-ray heating effect is enhanced significantly in the presence of an extended atmospheric layer with a temperature \,K above the accretion disk. We have derived simple analytic formulas for the disk heating by scattered X-ray photons using an approximate solution of the transfer equation by the Sobolev method. This approximation has a \,% accuracy in the range of X-ray photon energies \,keV.
19 pages, 8 figures, published in Astronomy Letters
References in corpus (1)
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