MC3D-simulating polarization maps and more

Details MC3D-simulating polarization maps and more MC3D-simulating polarization maps and more

Feb 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003spie.4843..524w&link_type=abstract

Polarimetry in Astronomy. Edited by Silvano Fineschi . Proceedings of the SPIE, Volume 4843, pp. 524-532 (2003).

Astronomy and Astrophysics

Astronomy

Scientific paper

MC3D is a three-dimensional, self-consistent continuum radiative transfer code. It can be used to determine the spatial temperature distribution in arbitrary dust/electron configurations, such as around young stellar objects or active galactic nuclei. Based on this temperature distribution, MC3D allows calculation of polarization maps, images, and spectral energy distributions. We present the numerical techniques applied in this code, describe its capabilities, and show instructive examples of previous applications.

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