WACCABI-A 2D Radiative Transfer Code for Stellar Winds in Cataclysmic Binaries

Details WACCABI-A 2D Radiative Transfer Code for Stellar Winds in Cataclysmic Binaries WACCABI-A 2D Radiative Transfer Code for Stellar Winds in Cataclysmic Binaries

Nov 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010aipc.1273..354s&link_type=abstract

17TH EUROPEAN WHITE DWARF WORKSHOP. AIP Conference Proceedings, Volume 1273, pp. 354-357 (2010).

Computer Science

Radiative Transfer, Accretion Disks, Hydrodynamics, Image Processing, Radiative Transfer, Scattering, Infall, Accretion, And Accretion Disks, Hydrodynamics, Image Processing

Scientific paper

We present a new 2D ray-tracing technique for computing the emergent spectra of winds originating from the surfaces of primary star and accretion disk in cataclysmic binaries. By using a highly modular approach, allowing easy modification and extension of the code, we self-consistently solve the pan-chromatic radiative transfer problem in moving media. Primary application of this code is to complement and to be used in conjunction with model atmosphere codes for stellar and accretion disk atmospheres and wind hydrodynamical models.

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