Abstract
Flow of matter in the immediate vicinity of a T Tauri type star with a constant dipole magnetic field on a two-dimensionalaxisymmetric computational grid is simulated. Within the framework of a nonstationary MHD approach, the interaction ofa jet, a partially ionized gas of the stellar corona, and a protoplanetary disk is considered. The model takes into accountthe degree of gas ionization, optically thin cooling, anisotropic thermal conductivity and viscosity. Numerical modeling isperformed using the free PLUTO package.
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.
