On the origin, acceleration and collimation of bipolar outflows and cosmic radio jets

Details On the origin, acceleration and collimation of bipolar outflows and cosmic radio jets On the origin, acceleration and collimation of bipolar outflows and cosmic radio jets

Mar 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992mnras.255..255c&link_type=abstract

Monthly Notices of the Royal Astronomical Society (ISSN 0035-8711), vol. 255, March 15, 1992, p. 255-260.

Astronomy and Astrophysics

Astronomy

20

Accretion Disks, Active Galactic Nuclei, Protostars, Radio Jets (Astronomy), Angular Momentum, Interstellar Magnetic Fields, Magnetohydrodynamic Flow, Maxwell Equation, Star Formation

Scientific paper

It is shown that it is possible to self-consistently obtain well-collimated bipolar outflows and radio jets from magnetized protostellar disks and accretion disks in active galactic nuclei. An analytical solution is given for the complete set of Euler-Maxwell equations both inside and outside the disk, and the solutions are appropriately matched on the disk surface. Disks with a power-law angular-momentum distribution are considered, and self-similarity is assumed in the radial direction. The solutions are obtained from the midplane of the disk until the outflow reaches the Alfven point.

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