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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
Abstract
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
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- Copyright © Astronomical Society of the Pacific 1999