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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
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

References

Balsara, D., 1995, J. ??m?. Phys., 121, 357 Google Scholar
Flebbo, O., Muenzel, S., Herold, H., Riffert, H., Ruder, H., 1994. Ap.J. 431, 754 Google Scholar
Foulkos, S., Haswell, ?., Murray, J., Rolfe, D., 2004. MNRAS, in pressGoogle Scholar
Kunze, S., Speith, R., Hessman, F., 2001, MNRAS. 322, 499 Google Scholar
Maddison, S., Humble, R., Murray, J., 2003, proc. of Scientific Frontiers in Research on Extrasolar Planets, ASP Conference Series 294. eds Deeming, & Seager, Google Scholar
Meglicki, Z., Wickramasinghe, D., Bicknell, G.V., 1995, MNRAS. 272, 717 Google Scholar
Monaghan, J., 1992, ARAA, 30, 543 Google Scholar
Morris, J., Monaghan, , 1997, J., J. ????. Phys., 136, 41 Google Scholar
Murray, J., 1996, MNRAS, 279, 402 Google Scholar
Ogilvie, G., 2003, MNRAS, 340, 969 Google Scholar
Steinmetz, M., 1996, MNRAS, 278, 1005 Google Scholar
Truss, M., Murray, J., Wynri, G., Edgar, R., 2000, MNRAS, 319, 467 Google Scholar
Truss, M., Murray, J., Wynn, , 2001, MNRAS, 324, L1 Google Scholar
Truss, M., Wynn, G.. Murray, J., Wynn, , King, A., 2002, MNRAS, 337, 1329, LIGoogle Scholar
Truss, M., Wynn, G., Wheatley, P., 2004, 347, 569 Google Scholar