Radiation-Accelerated Magnetized Jets

Mathematical modelling problem is stated for astrophysical jet outflows from the neighborhood of compact objects. Magnetohydrodynamical and radiation approaches explaining various properties of the outflows, are considered. Two model problems are presented within the framework of magnetohydrodynamical and radiation-magnetohydrodynamical statements in order to carry out self-consisted modeling of the processes ofjet’s formation, development and acceleration. Numerical research results are given for the problems under consideration. The results demonstrate formation and efficient radiation acceleration of a canalized jet outflow.

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