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Titlebook: Jets in Young Stellar Objects; Theory and Observati A. J. L. Fernandes,P. J. V. Garcia,J. J. G. Lima Book 2003 Springer Science+Business Me

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樓主: Croching
31#
發(fā)表于 2025-3-26 23:26:39 | 只看該作者
Thibaut Lery of fourteen years exists in their proposed tradition from the death of Yeats in 1939 to the premiere of Beckett’s En . in 1953. It follows that the plays of this period have been written out of a reading of a linear chronological tradition of modern Irish drama. This study examines the experimental
32#
發(fā)表于 2025-3-27 03:41:07 | 只看該作者
33#
發(fā)表于 2025-3-27 09:06:27 | 只看該作者
Daniel F.M. Folhaystems with too many variables to model easily but too few to make averaging a meaningful solution. Finally, there is the issue of non-stationarity. Non-stationary processes are those where the means, variance and co-variances change over time – often in unpredictable, stochastic ways. I offer sugge
34#
發(fā)表于 2025-3-27 09:29:05 | 只看該作者
35#
發(fā)表于 2025-3-27 15:41:29 | 只看該作者
36#
發(fā)表于 2025-3-27 20:17:42 | 只看該作者
37#
發(fā)表于 2025-3-27 22:33:03 | 只看該作者
38#
發(fā)表于 2025-3-28 05:33:21 | 只看該作者
Mhd Simulations of the Long-Term Evolution of a Dipolar Magnetosphere Surrounded By an Accretion Dis 30° to 55° depending on the ratio of the mass flow rates of disk wind and stellar wind. The maximum speed of the outflow is about the Keplerian speed at the inner disk radius. An axial jet forms during the first decades of rotations. However, this feature does not survive on the very long time scal
39#
發(fā)表于 2025-3-28 07:25:13 | 只看該作者
40#
發(fā)表于 2025-3-28 11:08:21 | 只看該作者
Three-Dimensional Simulations of Jets From Keplerian Disks: Stability Issuesf the outflow into the stretched, poloidal field lines of the distorted jet. This too has the effect of increasing the Alfvén speed and thereby reducing the Alfvénic Mach number. The jet is able to survive the onset of the more destructive . = 1 mode in this way.
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