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3D non-LTE radiative transfer: a new code and its application to γ2 Velorum

Published online by Cambridge University Press:  25 May 2016

Doris Folini  and
Rolf Walder
Doris Folini
Affiliation:
Institut of Astronomy, ETH Zürich, Switzerland
Rolf Walder
Affiliation:
Institut of Astronomy, ETH Zürich, Switzerland

Abstract

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A new approach to 3D optically thick non-LTE radiative transfer for moving media is presented. As a first application, we look at the ionization state of the colliding winds interaction zone between two stars.

Type
Part 3. Interaction of Wolf-Rayet stars and other hot massive stars with their environment: colliding winds and ring nebulae
Information
Symposium - International Astronomical Union , Volume 193: Wolf-Rayet Phenomena in Massive Stars and Starburst Galaxies , 1999 , pp. 352 - 353
Copyright
Copyright © Astronomical Society of the Pacific 1999 

References

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