- Portada
- Volume 80 - Année 2011
- 3D modelling of the massive star binary systems Eta Carinae, WR22, and WR140
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3D modelling of the massive star binary systems Eta Carinae, WR22, and WR140
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Anexidades
Abstract
Massive stars possess powerful stellar winds. Wind-wind collision in a massive star binary system generates a region of thermalized plasma which may emit prolifically at X-ray wavelengths. Results are presented from 3D adaptive-mesh refinement (AMR) hydrodynamical models which include radiative cooling and the radiative driving of the stellar winds. The models provide an exceptional insight into the turbulent nature of the wind-wind interaction regions. The X-ray emission from the hydrodynamical models is then calculated, allowing detailed comparisons with observational data. Preliminary results from investigations of Eta Carinae, WR22, and WR140 are discussed.
Para citar este artículo
Acerca de: E. R. Parkin
Institut d’Astrophysique et de Géophysique, Université de Liège, Belgium, and School of Physics and Astronomy, The University of Leeds, UK
Acerca de: J. M. Pittard
School of Physics and Astronomy, The University of Leeds, UK
Acerca de: M. F. Corcoran
CRESST and X-ray Astrophysics Laboratory, NASA/GSFC, USA, and Universities Space Research Association, USA
Acerca de: K. Hamaguchi
CRESST and X-ray Astrophysics Laboratory, NASA/GSFC, USA, and Department of Physics, University of Maryland, USA
Acerca de: I. R. Stevens
School of Physics and Astronomy, University of Birmingham, UK
Acerca de: E. Gosset
Institut d’Astrophysique et de Géophysique, Université de Liège, Belgium
Acerca de: G. Rauw
Institut d’Astrophysique et de Géophysique, Université de Liège, Belgium
Acerca de: M. De Becker
Institut d’Astrophysique et de Géophysique, Université de Liège, Belgium