持续
发表于 2025-3-23 12:06:47
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
发表于 2025-3-23 15:44:28
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hangdog
发表于 2025-3-23 18:51:07
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
发表于 2025-3-23 22:34:15
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Relinquish
发表于 2025-3-24 03:57:49
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注意到
发表于 2025-3-24 07:17:15
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Alpha-Cells
发表于 2025-3-24 12:14:10
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
抵制
发表于 2025-3-24 17:39:51
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Juvenile
发表于 2025-3-24 19:05:58
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gruelling
发表于 2025-3-25 03:10:55
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