On hydrodynamics of astrophysical jets. I - Basic equations

Details On hydrodynamics of astrophysical jets. I - Basic equations On hydrodynamics of astrophysical jets. I - Basic equations

May 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985mnras.214..161n&link_type=abstract

Monthly Notices of the Royal Astronomical Society (ISSN 0035-8711), vol. 214, May 15, 1985, p. 161-176. Research supported by th

Statistics

Computation

14

Astronomical Models, Computational Astrophysics, Hydrodynamic Equations, Interstellar Radiation, Plasma Acceleration, Plasma Jets, Accretion Disks, Black Holes (Astronomy), Galactic Nuclei, Gas Viscosity, Interstellar Gas, Optical Thickness

Scientific paper

A model for jet acceleration in the funnels of a geometrically thick, radiation-supported disc is constructed. The dynamics of matter lost from the funnels' surface is studied in a general relativistic background and by means of a fully hydrodynamical treatment, including viscosity. Hydrodynamic equations governing the gas flow are derived either for an optically thick or for an optically thin medium. The general behaviour of the solutions is discussed with particular emphasis to their existence and uniqueness.

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