Stellar atmospheres and stellar winds  

• The student can understand the main processes involved in radiation transfer • The student can interpret analytical and numerical solutions of radiation transfer, as described in the scientific literature, and can compare these methods with the ones illustrated in the course • The student can interpret the spectra of stellar atmospheres in function of temperature, gravity and chemical composition of the star • The student can understand the different physical causes for the onset of a stellar wind • The student can interpret observations of stellar winds using basic physical concepts, illustrated by means of simplified analytical equations or complex theoretical computer models
Presential
English
Stellar atmospheres and stellar winds
English

Funded by the European Union. Views and opinions expressed are however those of the author(s) only and do not necessarily reflect those of the European Union or HaDEA. Neither the European Union nor the granting authority can be held responsible for them. The statements made herein do not necessarily have the consent or agreement of the ASTRAIOS Consortium. These represent the opinion and findings of the author(s).