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A&A 417, 793-805 (2004)
DOI: 10.1051/0004-6361:20040017
The 2D continuum radiative transfer problem
Benchmark results for disk configurations
I. Pascucci1, S. Wolf1, 2, J. Steinacker1, 3, C. P. Dullemond4, Th. Henning1, G. Niccolini5, P. Woitke6 and B. Lopez51 Max-Planck-Institut für Astronomie, Königstuhl 17, 69117 Heidelberg, Germany
2 California Institute of Technology, 1201 East California Blvd, Mail Code 105-24, Pasadena, CA 91125, USA
3 Astrophysikalisches Institut und Universitäts-Sternwarte, Schillergässchen 2-3, 07745 Jena, Germany
4 Max-Planck-Institut für Astrophysik, Karl-Schwarzschild-Str. 1, 85741 Garching, Germany
5 Observatoire de la Côte d'Azur, Département Fresnel, UMR 6528, BP 4229, 06034 Nice Cedex 4, France
6 Zentrum für Astronomie und Astrophysik, TU Berlin, Hardenbergstraße 36, 10623 Berlin, Germany
(Received 26 July 2002 / Accepted 2 January 2004)
Abstract
We present benchmark problems and solutions for the continuum radiative
transfer (RT) in a 2D disk configuration.
The reliability of three Monte-Carlo and two grid-based codes is tested
by comparing their results for a set of well-defined cases which differ
for optical depth and viewing angle.
For all the configurations, the overall shape of the resulting temperature
and spectral energy distribution is well reproduced.
Key words: radiative transfer -- stars: circumstellar matter -- methods: numerical
Offprint request: I. Pascucci, pascucci@mpia-hd.mpg.de
© ESO 2004
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