A wind-type model for the generation of astrophysical jets

Details A wind-type model for the generation of astrophysical jets A wind-type model for the generation of astrophysical jets

Feb 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984apj...277l..35f&link_type=abstract

Astrophysical Journal, Part 2 - Letters to the Editor (ISSN 0004-637X), vol. 277, Feb. 15, 1984, p. L35-L39. Research supported

Astronomy and Astrophysics

Astrophysics

26

Accretion Disks, Astronomical Models, Galactic Nuclei, Plasma Dynamics, Plasma Jets, Stellar Winds, Active Galactic Nuclei, Collimation, Hydrodynamics, Magnetohydrodynamic Waves, Plasma Acceleration, Solar Wind, Supersonic Flow, Two Dimensional Flow

Scientific paper

Wind-type solutions are discussed for the generation of astrophysical jets from active galactic nuclei and stellar sources such as those associated with SS433 and protostellar objects. Acceleration, collimation, and morphology are consistently interpreted in terms of a flow starting from the galactic or stellar core inside the "throat" of a thick accretion disk.

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