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. http://resolver.caltech.edu/CaltechAUTHORS:20160708-080025018
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Abstract
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 | |||||||||
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| Additional Information: | © 2016 EAS, EDP Sciences. | |||||||||
| Record Number: | CaltechAUTHORS:20160708-080025018 | |||||||||
| Persistent URL: | http://resolver.caltech.edu/CaltechAUTHORS:20160708-080025018 | |||||||||
| 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: http://dx.doi.org/10.1051/eas/1575030 | |||||||||
| Usage Policy: | No commercial reproduction, distribution, display or performance rights in this work are provided. | |||||||||
| ID Code: | 68906 | |||||||||
| Collection: | CaltechAUTHORS | |||||||||
| Deposited By: | Tony Diaz | |||||||||
| Deposited On: | 09 Jul 2016 04:50 | |||||||||
| Last Modified: | 30 Aug 2017 21:07 |
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