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A two-dimensional hydrodynamic numerical model is extended and applied to simulate the interaction between stellar winds and the interstellar medium (ISM). In particular, the stellar wind evolution of O- and B-type stars is calculated. First, the evo
Externí odkaz:
http://hdl.handle.net/10394/9719
Thesis (MSc (Space Physics))--North-West University, Potchefstroom Campus, 2011. A two-dimensional hydrodynamic numerical model is extended and applied to simulate the interaction between stellar winds and the interstellar medium (ISM). In particular
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=od______1399::e44d4e4d33ef155b12ab06bdff2aea96
https://hdl.handle.net/10394/9719
https://hdl.handle.net/10394/9719