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Hydro dynamical Evolution of Circumbinary Accretion Disks

Published online by Cambridge University Press:  12 April 2016

M. Różyczka  and
G. Laughlin
M. Różyczka
Affiliation:
Warsaw University Observatory, Aleje Ujazdowskie 4, 00–478 Warszawa, Poland Department of Physics, University of Michigan, Ann Arbor, MI 48109–1120, USA
G. Laughlin
Affiliation:
Department of Physics, University of Michigan, Ann Arbor, MI 48109–1120, USA

Abstract

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SPH simulations of circumbinary accretion disks are verified with the help of a grid-based Eulerian code. The phenomenon of pulsed accretion flow through the central gap is confirmed.

Type
Part 15. Poster Papers
Information
International Astronomical Union Colloquium , Volume 163: Accretion Phenomena and Related Outflows , 1997 , pp. 792 - 793
Copyright
Copyright © Astronomical Society of the Pacific 1997

References

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Marcy, G. & Butler, P. 1996, WWW server, http://cannon.sfsu.edu/ williams/planetsearch.html Google Scholar
Różyczka, M.& Spruit, H. 1993, ApJ, 417, 677 Google Scholar