Effects of local thermodynamics and of stellar mass ratio on accretion disc stability in close binaries

DOI10.1002/ASNA.200811243zbMath1181.85028OpenAlexW2094181818MaRDI QIDQ3401341

G. Lanzafame

Publication date: 29 January 2010

Published in: Astronomische Nachrichten (Search for Journal in Brave)

Full work available at URL: https://doi.org/10.1002/asna.200811243

zbMATH Keywords

accretionaccretion disksbinaries: closecataclysmic variablesnovaestars: dwarf novae

Mathematics Subject Classification ID

Galactic and stellar structure (85A15) Hydrodynamic and hydromagnetic problems in astronomy and astrophysics (85A30) Stability and instability of geophysical and astrophysical flows (76E20)

Related Items (1)

Implicit integrations for SPH in semi-Lagrangian approach: application to the accretion disc modeling in a microquasar

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