Cold super-fast MHD winds from rapid rotators.

Details Cold super-fast MHD winds from rapid rotators. Cold super-fast MHD winds from rapid rotators.

Jan 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991srtoh..11..121t&link_type=abstract

Sci. Rep. Tôhoku Univ., Eighth Ser., Vol. 11, Nos. 2/3, p. 121 - 123

Computer Science

Scientific paper

Active galactic nuclei (AGNs) and quasars dissipate energy in the form of a relativistic magnetized jet. The author studies relativistic ideal magnetohydrodynamical (MHD) winds in a stationary and axisymmetric magnetosphere of a rapidly rotating compact object without gravitational and pressure effects. He analyses regularity conditions of MHD flows at the Alfven point and fast magnetosonic point, where the poloidal velocity equals to the speed of the Alfven wave or the fast magnetosonic wave.

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