Titlebook: Angular Momentum Evolution of Young Stars; S. Catalano,J. R. Stauffer Book 1991 Springer Science+Business Media Dordrecht 1991 CCD.dynamic

持續(xù)

Differential Rotation of Fully Convective Pre-Main Sequence Starsnsport coefficients. The models have a large scale circulation and differential rotation. Models with standard isotropic transport also have circulation and differential rotation; the circulation being driven by the latitudinal variation of convective and radiative heat flux in rotating stars in an

Essential

hangdog

Multifrequency Monitoring of RU Lupi: Observational Results and a Modelults and a first attempt of their interpretation. The various phenomena observed in RU Lupi can be explained in term of a disk accretion onto an young star with a moderately strong global magnetic field. The role of axial rotation is also discussed.

languid

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Alpha-Cells

Rotational Velocities of Stars in Open Clusters: The Time Dependence Revisitedence of stellar rotation. The shape of the Vsini distribution is an extremely sensitive function of the α index of the braking law (dV/dt = -AV.). The comparison of Hyades + Praesepe and Pleiades observations favours the value . = 2. The Vsini distributions could not be reproduced with . = 3, the va

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Juvenile

gruelling