Spectral synthesis of circumstellar disks - application to white dwarf debris disks

Details Spectral synthesis of circumstellar disks - application to white dwarf debris disks Spectral synthesis of circumstellar disks - application to white dwarf debris disks

2009-05-04

arxiv.org/abs/0905.0329v1

J.Phys.Conf.Ser.172:012060,2009

Astronomy and Astrophysics

Astrophysics

Solar and Stellar Astrophysics

4 pages, 4 figures, to appear in: Proceedings of the 16th European Workshop on White Dwarfs

Scientific paper

10.1088/1742-6596/172/1/012060

Gas and dust disks are common objects in the universe and can be found around various objects, e.g. young stars, cataclysmic variables, active galactic nuclei, or white dwarfs. The light that we receive from disks provides us with clues about their composition, temperature, and density. In order to better understand the physical and chemical dynamics of these disks, self-consistent radiative transfer simulations are inevitable. Therefore, we have developed a 1+1D radiative transfer code as an extension to the well-established model atmosphere code \verb!PHOENIX!. We will show the potential of the application of our code to model the spectra of white dwarf debris disks.

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