A Caltech Library Service

Continuum radiative transfer Modeling of Sagittarius B2

Schmiedeke, A. and Schilke, P. and Möller, Th. and Sánchez-Monge, Á. and Bergin, E. and Comito, C. and Csengeri, T. and Lis, D. C. and Molinari, S. and Qin, S. L. and Rolffs, R. (2016) Continuum radiative transfer Modeling of Sagittarius B2. In: Conditions and impact of star formation: from lab to space : in Memory of Charles H. Townes. EAS Publications Series. No.75-76. EDP Sciences , Les Ulis, France, pp. 171-174. ISBN 978-2-7598-2022-1.

[img] PDF - Published Version
See Usage Policy.


Use this Persistent URL to link to this item:


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 free-free 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).

Item Type:Book Section
Related URLs:
URLURL TypeDescription
Schilke, P.0000-0003-2141-5689
Lis, D. C.0000-0002-0500-4700
Additional Information:© 2016 EAS, EDP Sciences.
Series Name:EAS Publications Series
Issue or Number:75-76
Record Number:CaltechAUTHORS:20160708-080025018
Persistent URL:
Official Citation:Continuum radiative transfer Modeling of Sagittarius B2 A. Schmiedeke, P. Schilke, Th. Möller, Á. Sánchez-Monge, E. Bergin, C. Comito, T. Csengeri, D.C. Lis, S. Molinari, S.L. Qin and R. Rolffs EAS Publications Series, 75-76 (2015) 171-174 DOI:
Usage Policy:No commercial reproduction, distribution, display or performance rights in this work are provided.
ID Code:68906
Deposited By: Tony Diaz
Deposited On:09 Jul 2016 04:50
Last Modified:09 Mar 2020 13:19

Repository Staff Only: item control page