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Hydrodynamic Modelling of Accretion Flows

Published online by Cambridge University Press:  22 February 2018

J. R. Murray,
M. R. Truss,
S. B. Foulkes,
C. A. Haswell and
K. J. Manson
J. R. Murray
Affiliation:
Swinburne University of Technology, Australia
M. R. Truss
Affiliation:
University of St Andrews, UK
S. B. Foulkes
Affiliation:
Open University, Milton Keynes, UK
C. A. Haswell
Affiliation:
Open University, Milton Keynes, UK
K. J. Manson
Affiliation:
Swinburne University of Technology, Australia

Abstract

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In the proceedings of this, and of several recent close binary conferences, there have been several contributions describing smoothed particle hydrodynamics simulations of accretion disks. It is opposite therefore to review the numerical scheme itself with emphasis on its advantages for disk modelling, and the methods used for modelling viscous processes.

Resumen

Resumen

En estas memorias y en algunas otras de conferencias recientes sobre binarias cercanas hay varias contribuciones describiendo simulaciones hidrodinámicas de partículas suaves de discos de acreción. Es el momento adecuado de revisar el esquema numérico en sí mismo enfatizando sus ventajas para el modelado de discos y los métodos usados para el modelado de procesos viscosos.

Keywords

AccretionAccretion Disks — BinariesClose — LineProfiles — XRaysBinaries — Hydrodynamics

Information

Type
The Contributed Papers
Information
International Astronomical Union Colloquium , Volume 194: Compact binaries in the galaxy and beyond , 2004, pp. 166 - 168
Copyright
Copyright © Instituto de astronomia/revista mexicana de astronomίa y astrofίsica 2004

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