Abstract
We present the results of detailed numerical calculations of the transport of radiation in spherical accretion flows onto compact objects. We show that Comptonization by the electron bulk motion should not be neglected in computing the X-ray spectra of accreting compact objects and demonstrate the importance of retaining the terms in the radiative transfer equation that are at least second-order in the electron bulk velocity.
Talk to us
Join us for a 30 min session where you can share your feedback and ask us any queries you have
Disclaimer: All third-party content on this website/platform is and will remain the property of their respective owners and is provided on "as is" basis without any warranties, express or implied. Use of third-party content does not indicate any affiliation, sponsorship with or endorsement by them. Any references to third-party content is to identify the corresponding services and shall be considered fair use under The CopyrightLaw.