CONTINUUM RADIATIVE TRANSFER MODELING OF SAGITTARIUS B2.

We present results from radiative transfer modeling of the continuum emission towards Sagittarius B2 (hereafter Sgr B2). We have developed a radiative transfer framework - Pandora - that employs RADMC-3D (Dullemond 2012) for a self-consistent determination of the dust temperature. With this pipeline, we have set-up a single model that consistently reproduces the thermal dust and freefree continuum emission of Sgr B2 spanning four orders of magnitude in spatial scales (0.02-45 pc) and two orders of magnitude in frequency (20-4000 GHz). [ABSTRACT FROM AUTHOR]