Hostname: page-component-848d4c4894-pjpqr Total loading time: 0 Render date: 2024-06-25T20:41:47.268Z Has data issue: false hasContentIssue false
  • English
  • Français

HDUST3 — A chemically realistic, 3-D, NLTE radiative transfer code

Published online by Cambridge University Press:  28 July 2017

Alex C. Carciofi ,
Jon E. Bjorkman  and
Janos Zsargó
Alex C. Carciofi
Affiliation:
Instituto de Astronomia, Geofísica e Ciências Atmosféricas, Universidade de São Paulo, Rua do Matão 1226, Cidade Universitária, 05508-900 São Paulo, SP, Brazil email: carciofi@usp.br
Jon E. Bjorkman
Affiliation:
Ritter Observatory, Dept. of Phys. & Astron., MS 113, Univ. of Toledo, Toledo, OH 43606
Janos Zsargó
Affiliation:
Escuela Superior de Física y Matemática. Instituto Politécnico Nacional. Av. Instituto Politécnico Nacional, Edificio 9, C.P. 07738, DF. México
Rights & Permissions [Opens in a new window]

Abstract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

HDUST is a 3D, NLTE radiative transfer code based on the Monte Carlo method. We report on recent advancements on the code, which is now capable of handling He and other elements in the NLTE regime and in 3D configurations. In this contribution we show initial comparisons with CMFGEN, made with spherical wind models composed of H + He.

Keywords

methods: numericalradiative transfer
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 12 , Symposium S329: The Lives and Death-Throes of Massive Stars , November 2016 , pp. 390
Copyright
Copyright © International Astronomical Union 2017 

References

Carciofi, A. C., Bjorkman, J. E., & Magalhães, A. M., 2004, ApJ, 604, 238 Google Scholar
Carciofi, A. C., & Bjorkman, J. E., 2006, ApJ, 639, 1081 Google Scholar