Numerical Simulations Of Radiatively Inefficient Flows Accreting Onto Radiatively Efficient Black Hole Objects

Details Numerical Simulations Of Radiatively Inefficient Flows Accreting Onto Radiatively Efficient Black Hole Objects Numerical Simulations Of Radiatively Inefficient Flows Accreting Onto Radiatively Efficient Black Hole Objects

Sep 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006head....9.0704p&link_type=abstract

American Astronomical Society, HEAD meeting #9, #7.04; Bulletin of the American Astronomical Society, Vol. 38, p.350

Astronomy and Astrophysics

Astronomy

Scientific paper

I present results from hydrodynamical simulations of gas dynamics
outside luminous accretion disks in quasars. The goal of these
simulations is to study how radiative heating and radiation pressure can
affect the large-scale flow properties such as the mass supply and
outflow rate.

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