Steady accretion-jet flows

Details Steady accretion-jet flows Steady accretion-jet flows

Oct 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989kfnt....5...37m&link_type=abstract

Kinematika i Fizika Nebesnykh Tel (ISSN 0233-7665), vol. 5, Sept.-Oct. 1989, p. 37-42. In Russian.

Astronomy and Astrophysics

Astronomy

Astronomical Models, Black Holes (Astronomy), Rotating Matter, Stellar Mass Accretion, Axisymmetric Flow, Steady Flow, Thermal Conductivity

Scientific paper

Models are constructed for steady axisymmetric flow containing jet bipolar streams with accretion of rotating matter in areas adjacent to the equatorial plane. The most effective model is jet outflow of matter, in which the thermal diffusivity of accreting matter has a value close to that of its kinematic viscosity, and kinematic viscosity and temperature conduction rapidly increase with temperature.

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