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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2- and 3-D Simulations of Magnetocentrifugal Disk-Winds: Acceleration and Stabilityct launching conditions on the disk, such as the distributions of magnetic flux and mass ejection rate, are poorly known. They could be constrained from observations at large distances, provided that a robust model is available to link the observable properties of the jets and winds at the large dis

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Hh 111 Stis Observations and Their Analysis Using Analytical and Numerical Modelsupersonic proper motions. These structures, we believe, are the result of a variable ejection from the source, which leads to the formation of . or small bowshock within the jet beam. In this paper we present a long-slit spectrum of Herbig-Haro object HH 111 obtained with STIS and an interpretation

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Bravura

Three-Dimensional Simulations of Jets From Keplerian Disks: Stability Issues. We investigate the outflow that arises from a magnetized accretion disk that is initially in hydrostatic balance with its surrounding cold corona. Our simulations show that jets maintain their long-term stability through a self-limiting process wherein the average Alfvénic Mach number within the j

alabaster

Mhd Simulations of Jets From Accretion Disksly. Although it was considered that this kind of simulations only shows the transient phenomena of jets, we found that the outflow and accretion flow reached a quasi-steady state by performing a long-term calculation in a large calculation region. Though the final stage is not exactly the steady sta

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Transfusion

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