Radiative transfer in dusty discs: models of bipolar flow sources.

Details Radiative transfer in dusty discs: models of bipolar flow sources. Radiative transfer in dusty discs: models of bipolar flow sources.

Dec 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992dudi.work..141e&link_type=abstract

"Dusty Discs, Proceedings of the 9th RAL Workshop on Astronomy and Astrophysics. Edited by P.M. Gondhalekar.

Astronomy and Astrophysics

Astrophysics

Scientific paper

The author presents a generalisation of the method of Efstathiou and
Rowan-Robinson (1991) for modelling low-mass protostars that takes into
account a distribution of grain species and sizes. The method includes
treatment of multiple scattering from grains. The authors apply this
method to protostellar systems which are in the bipolar flow phase.

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