Computer modeling of W Serpentis binaries through the use of smoothed particle hydrodynamics.

Details Computer modeling of W Serpentis binaries through the use of smoothed particle hydrodynamics. Computer modeling of W Serpentis binaries through the use of smoothed particle hydrodynamics.

Jul 1996

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1996iappp..64....9n&link_type=abstract

I.A.P.P.P. Commun., No. 64, p. 9 - 13

Other

Close Binaries: Numerical Simulations, Close Binaries: Hydrodynamics, Close Binaries: Mass Transfer

Scientific paper

W Serpentis stars are long-period close binary star systems exhibiting rapid-phase mass transfer from a Roche lobe-filling star to another star which is considerably within the limits of its Roche lobe. Accretion disks for three such stars, V356 Sgr, V453 Sco, and W Ser itself, were modeled using a Smoothed Particle Hydrodynamics (SPH) program written by Simpson. SPH allows for the modeling of media that interact non-gravitationally; it is useful in the study of non-ideal gases.

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