Hostname: page-component-848d4c4894-nr4z6 Total loading time: 0 Render date: 2024-05-15T01:51:42.323Z Has data issue: false hasContentIssue false
  • English
  • Français

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

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

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

Artymowicz, P. & Lubow, S.H. 1996, ApJ, in printGoogle Scholar
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