Spectral formation in compact X-ray sources

A method is described for calculating the transfer of X-rays through gas that is optically thick to Compton scattering. The method permits the simultaneous solution of the radiation-dominated temperature and ionization structure of the medium as well as the effects of incoherent Compton scattering of photons. Self-consistent results are obtained for idealized models of compact X-ray sources, represented as point sources of continuum X-rays surrounded by spherical shells of gas, demonstrating the range of spectral features that might result from such optically thick transfer. Some implications for the analysis of X-ray spectra of galactic X-ray sources are discussed.