W. Hummel, K. Horne, T. R. Marsh, Janet H. Wood
Abstract
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Abstract We derive the temperature and density structure of the accretion disk of the dwarf nova U Gem in quiescence from 3D radiative line and continuum transport calculations of a differentially rotating disk.
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Abstract We derive the temperature and density structure of the accretion disk of the dwarf nova U Gem in quiescence from 3D radiative line and continuum transport calculations of a differentially rotating disk.
Key concepts: Dwarf nova, Physics, Astrophysics, Accretion disc, Radiative transfer, Intermediate polar, Accretion (finance), Line (geometry)