Hydrodynamical Models of Accretion Disks in SU UMa Systems

• Autorzy: Kornet K. , Różyczka M.
• Języki publikacji: EN

Abstrakty

EN

We numerically test the mode-coupling model (Lubow 1991a) of tidal instability in SU UMa systems. So far, all numerical models confirming it have been based on SPH codes and isothermal equation of state. In our paper we present Eulerian models, using both isothermal approximation and the full energy equation. We also investigate influence of different ways of mass transfer. While isothermal models behave similarly to SPH simulations, the behavior of models with full energy equation is quite different, and the mode-coupling model is not confirmed in this case.

Słowa kluczowe

EN

novae; cataclysmic variables; accretion; accretion disks

• Wydawca: Copernicus Foundation for Polish Astronomy
• Czasopismo: Acta Astronomica
• Rocznik: 2000
• Tom: Vol. 50, No. 2
• Strony: 163--175
• Opis fizyczny: Bibliogr. 11 poz., wykr., zdj.

Twórcy

autor

Kornet K.

• N. Copernicus Astronomical Center,00-716 Warszawa, Bartycka 18

autor

Różyczka M.

• N. Copernicus Astronomical Center,00-716 Warszawa, Bartycka 18

Bibliografia

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• Murray, J.R. 1996, MNRAS, 279, 402.
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• Smak, J.I. 1999, "Disk Instabilities in Close Binary Systems. 25 Years of the Disk-Instability Model", Eds. S. Mineshige, and J.C. Wheeler, Frontiers Science Series No. 26 (Universal Academy Press, Inc.) p. 1.
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