The DYNAMO group aims to promote the development of collaborative projects in stellar physics. More specifically, our research focuses on the modeling and understanding of magnetized and unmagnetized fluid flows that affect transport processes in stellar interiors. DYNAMO brings together a wide range of skills in theory, numerical modeling and observational techniques to provide the most complete possible description of how stars function from birth to death. Members are involved in developing innovative research projects, organizing research (workshops, conferences, calls for proposals, etc.), collective tasks and teaching at different levels.
More at : https://dynamos.obspm.fr
