Astronomy and Astrophysics – Astronomy
Scientific paper
May 2009
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009aas...21442801g&link_type=abstract
American Astronomical Society, AAS Meeting #214, #428.01; Bulletin of the American Astronomical Society, Vol. 41, p.697
Astronomy and Astrophysics
Astronomy
Scientific paper
We compare smoothed particle hydrodynamics (SPH) simulations of artificially tilted and non-tilted, quasi-static accretion disks in Cataclysmic Variable systems. The accretion disks are simulated in 3D with 100,000 particles to show resolution in the z-direction. For these simulations, we assume a secondary-to-primary mass ratio q=0.4 and low mass transfer rates. Comparing the densities, internal energy emissions, and velocities within each disk and between disks tilted twenty degrees and non-tilted disks, we seek to identify significant features and the source to negative superhumps. We present face-on and edge-on accretion disks. We would like to acknowledge grants from the AAS small research grant and the UCF/UF Space Research Initiative.
Guasch Mark H.
Montgomery Martin
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