HIGHLIGHTS
- who: Ouazzani R.-M. and collaborators from the , Meudon, France Stellar Astrophysics Centre, Department of Physics and, Aarhus University, Ny Munkegade , have published the research work: γ Doradus stars as a test of angular momentum transport models, in the Journal: (JOURNAL)
- what: The authors show that the stellar buoyancy radius can be used as reliable evolution indicator for field stars on the main sequence. The authors show clear disagreement between the near-core rotation rates measured in the sample and the rotation rates obtained from the evolutionary models including rotationally induced transport of angular momentum following . . .
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