Influence of Rotation Velocity Gradient on Line Profiles of Accretion Discs of CVs

0388455 - ASÚ 2013 RIV GB eng C - Konferenční příspěvek (zahraniční konf.)
Korčáková, D. - Nagel, T. - Werner, K. - Suleimanov, V. - Votruba, Viktor
Influence of Rotation Velocity Gradient on Line Profiles of Accretion Discs of CVs.
From Interacting Binaries to Exoplanets: Essential Modeling Tools. Cambridge: Cambridge University Press, 2012 - (Richards, M.), s. 255-256. Proceedings of the International Astronomical Union, IAU S282. ISBN 9781107019829. ISSN 1743-9213.
[Symposium of the International Astronomical Union /282./. Tatranská Lomnica (SK), 18.07.2011-22.07. 2011]
Grant CEP: GA ČR(CZ) GP205/09/P476
Výzkumný záměr: CEZ:AV0Z10030501
Klíčová slova: rotation * mass loss * hydrodynamics
Kód oboru RIV: BN - Astronomie a nebeská mechanika, astrofyzika

We show the influence of the Keplerian velocity shear on the line profiles of cataclysmic variable discs. The complete disc structure is taken into account. The radial disc structure follows the alpha disc approximation. Based on this assumption, the vertical structure is computed using the detailed non-LTE code AcDc. The obtained opacities and source functions are interpolated in the 2D grid, where the radiative transfer is calculated with the inclusion of the velocity field gradient.
Trvalý link: http://hdl.handle.net/11104/0217351