Abstract
Abstract Gas dynamic features of slowly rotating axially symmetric gas accretion on to a gravitating centre are investigated. The process of flow restructuring is studied as the angular velocity of accreting matter approaches the Keplerian angular velocity. For spherically symmetric accretion the conditions are found of the existance of a steady-state state supersonic solution for various extertnal boundary conditions. A numerical study is performed on the basis of the Lax-Friedrichs-type second-order numerical scheme with an implicit approximation of the term in the Euler equations.
Sign-in/Register to access full text options 
Talk to us
Join us for a 30 min session where you can share your feedback and ask us any queries you have
Schedule a callDisclaimer: 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.
