DUSTY: a Publicly Available Code for Modeling Dust Emission

Details DUSTY: a Publicly Available Code for Modeling Dust Emission DUSTY: a Publicly Available Code for Modeling Dust Emission

Mar 2000

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2000aspc..196...77n&link_type=abstract

Thermal Emission Spectroscopy and Analysis of Dust, Disks, and Regoliths, Proceedings of a meeting held at at The Lunar and Plan

Astronomy and Astrophysics

Astrophysics

25

Scientific paper

We have developed the code DUSTY, publicly available at http://www.pa.uky.edu/~moshe/dusty/, for solving the radiative transfer problem in a dusty astrophysical environment. The code can handle both spherical and planar geometries and offers many options for input radiation, dust types and density distributions. It has a flexible, user-friendly input / output and has been tested on a variety of existing platforms. To be placed on DUSTY's mailing list send an e-mail to moshe@pa.uky.edu.

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