Article contents
Hydrodynamic modeling of accretion shocks on a star with radiative transport and a chromospheric model
Published online by Cambridge University Press: 13 February 2013
Abstract
Accretion flows on the surface of a star is modeled using a high resolution hydrodynamic 1D ALE code (ASTROLABE) coupled to radiative transfer and line cooling, along with a model for the acoustic heating of the chromospheric plasma.
- Type
- Research Article
- Information
- Copyright
- © The Author(s) 2013
References
Références
- 4
- Cited by