Blobby accretion in magnetic cataclysmic variables

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dc.creatorHalevin, A. V.
dc.creatorAndronov, I. L.
dc.creatorShakhovskoy, N. M.
dc.creatorKolesnikov, S. V.
dc.creatorOstrova, N. I.
dc.date2003-01-29
dc.date.accessioned2026-07-07T02:07:21Z
dc.date.available2026-07-07T02:07:21Z
dc.descriptionThe processes of accretion of the gaseous blobs with different masses and densities onto strongly magnetized white dwarfs in the systems of polars have been modeled. We have proved that shot noise in blue wavelengths represents accretion of the smaller and denser blobs than in redder wavelengths. Using combined "smooth particle hydrodynamics - drag force" model, we have predicted a shape of the accretion stream and active regions on the white dwarf surface.
dc.description7 pages 6 figures. To appear in the Proceedings of the IAU Colloquium 190 `Magnetic Cataclysmic Variables', 8-13 December 2002, Cape Town, South Africa
dc.identifierhttps://arxiv.org/abs/astro-ph/0301570
dc.identifierhttp://arxiv.org/abs/astro-ph/0301570
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/5669
dc.subjectAstrophysics
dc.titleBlobby accretion in magnetic cataclysmic variables
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