Non adiabatic self-consistent spherical accretion

Details Non adiabatic self-consistent spherical accretion Non adiabatic self-consistent spherical accretion

Oct 1982

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982ans..conf..146w&link_type=abstract

In Max-Planck Inst. Phys. and Astrophys. Accreting Neutron Stars p 146-149 (SEE N83-15179 05-88)

Computer Science

Numerical Analysis

Black Holes (Astronomy), Deposition, Energetic Particles, Energy Transfer, Luminosity, Spherical Plasmas, Eddington Approximation, Mathematical Models, Numerical Analysis, Radiant Flux Density

Scientific paper

New solutions for spherical accretion onto a black hole are presented.
The solutions are self consistent so that the infalling gas itself emits
the radiation which controls its thermal profile. These solutions
involve high accretion rates, yielding high luminosities.

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