Hostname: page-component-586b7cd67f-2brh9 Total loading time: 0 Render date: 2024-11-30T16:18:42.713Z Has data issue: false hasContentIssue false
  • English
  • Français

Simulations of disks in binary systems using parallelized SPH to reach extreme spatial resolution

Published online by Cambridge University Press:  26 May 2016

D. Molteni ,
F. Fauci ,
G. Gerardi  and
M. A. Valenza
D. Molteni
Affiliation:
Dipartimento di Fisica e Tecnologie Relative, Universita' di Palermo, Italy
F. Fauci
Affiliation:
Dipartimento di Fisica e Tecnologie Relative, Universita' di Palermo, Italy
G. Gerardi
Affiliation:
Dipartimento di Fisica e Tecnologie Relative, Universita' di Palermo, Italy
M. A. Valenza
Affiliation:
Dipartimento di Fisica e Tecnologie Relative, Universita' di Palermo, Italy

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.

Results of 3D numerical simulations of the gas transfer in close binary systems show that it is possible the production of accretion streams having low specific angular momentum in a region close to the accreting star. These streams are mainly placed above the orbital disc. The eventual formation of such bulges and shock heated flows is interesting in the context of advection dominated solutions and for the explanation of spectral properties of the Black Hole candidates in binary systems. We set up a parallelized version of 3D S.P.H. code, using domain decomposion. with increasing spatial resolution around the compact star.

Type
Posters
Information
Symposium - International Astronomical Union , Volume 208: Astrophysical Supercomputing using Particle Simulations , 2003 , pp. 427 - 428
Copyright
Copyright © Astronomical Society of the Pacific 2003 

References

Frank, J., King, A., Raine, D., 1992, Accretion Power in Astrophysics, Cambridge Univ. Press, Cambridge Google Scholar
Chakrabarti, S.K., Titarchuk, L.G., 1995, ApJ, 455, 623 Google Scholar
Molteni, D., Kuznetsov, O. A., Bisikalo, D. V., Boyarchuk, A. A., 2001, MNRAS, 327, 1103 Google Scholar