Generating Eclipsing CV RVs from SPH Numerical Simulations

Details Generating Eclipsing CV RVs from SPH Numerical Simulations Generating Eclipsing CV RVs from SPH Numerical Simulations

May 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010aas...21642702s&link_type=abstract

American Astronomical Society, AAS Meeting #216, #427.02; Bulletin of the American Astronomical Society, Vol. 41, p.840

Astronomy and Astrophysics

Astronomy

Scientific paper

We present SPH numerically simulated face-on and edge-on accretion disks that show variation in speeds within the disk. In our simulations, we assume a non-magnetic CV system with mass ratio q=0.4 and primary mass M1=0.8 solar masses. We generate artificial radial velocity curves of the system in eclipse. We consider various disk shapes and the various different speeds on the rim of the disk. In this work, we show how we obtained the artificial RV curves.

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