Virtual Astrophysical Jets Theory Versus Observations

These proceedings are the result of a three-day meeting held in Oogliani (Italy), on October 2-4 2003, whose title was "VIrtual Astrophysical Jets 2003". Our goal in convening this meeting was to gather some of the scientists among the most active in the field of numerical simulations and...

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Bibliographic Details
Other Authors: Massaglia, Silvano (Editor), Bodo, Gianluigi (Editor), Rossi, P. (Editor)
Format: eBook
Language:English
Published: Dordrecht Springer Netherlands 2004, 2004
Edition:1st ed. 2004
Subjects:
Online Access:
Collection: Springer Book Archives -2004 - Collection details see MPG.ReNa
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245 0 0 |a Virtual Astrophysical Jets  |h Elektronische Ressource  |b Theory Versus Observations  |c edited by Silvano Massaglia, Gianluigi Bodo, P. Rossi 
250 |a 1st ed. 2004 
260 |a Dordrecht  |b Springer Netherlands  |c 2004, 2004 
300 |a XV, 269 p. 85 illus  |b online resource 
505 0 |a Observational Properties of Jets in Active Galactic Nuclei -- AGN Jet Modeling: Setting the Stage -- Interpreting the Observations of Herbig-Haro Jets -- Virtual Versus Real Jets: New Clues from the Hubble Space Telescope -- The Origin of Jets from Young Stars: Steady State Disk Wind Models Confronted to Observations -- Steady and Time-Dependent MHD Modelling of Jets -- The Efficiency of the Magnetic Acceleration in Relativistic Jets -- MHD Outflows from Hot Coronae -- Virtual Jets: From Self-Similar to Numerical Solutions -- MHD Accretion-Ejection Flows -- On the MHD Acceleration of Astrophysical Jets -- MHD Simulations of Crab’s Jet and Torus -- The Stability Properties of Astrophysical Jets -- How Can Jets Survive MHD Instabilities? -- Stability of Relativistic Hydrodynamical Planar Jets: Linear and Nonlinear Evolution of Kelvin-Helmholtz Modes -- Entrainment and Deceleration of Relativistic Jets -- MHD Simulations of Relativistic Jets -- Computation of X-Ray Blazar Light Curves using RHD Simulations -- Effects of the Magnetic Field on the H? Emission from Jets -- Properties of Knots in Cooling Stellar Jets -- Are Astrophysical Shear Flows Able to Heat Themselves? -- Astrophysical Jet Simulations: Comparing Different Numerical Methods -- Axisymmetric Simulations of Pulsar Wind Nebulae with a New Central-Type Scheme for Relativistic MHD -- Simulating Magnetized Jets -- Experiments and Numerical Simulations on the Mid-Term Evolution of Hypersonic Jets -- Jet Propagation Through Irregular Media and the Impact of Lobes on Galaxy Formation -- Numerical Simulations of the Interaction of Jets with the Intracluster Medium -- Large Scale Simulations of the Jet-IGM Interaction -- The Environment of YSO Jets 
653 |a Astronomy, Cosmology and Space Sciences 
653 |a Astrophysics 
653 |a Astronomy 
700 1 |a Bodo, Gianluigi  |e [editor] 
700 1 |a Rossi, P.  |e [editor] 
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520 |a These proceedings are the result of a three-day meeting held in Oogliani (Italy), on October 2-4 2003, whose title was "VIrtual Astrophysical Jets 2003". Our goal in convening this meeting was to gather some of the scientists among the most active in the field of numerical simulations and modelling of astrophysi­ cal jets. For keeping the participants close to the "real world", we also invited a few observers to give up-to-date reviews outlining the state-of-the-art of jet observations. The principal aim of the meeting was thus to present and critically discuss the state-of-the-art numerical simulations, analytical models and laboratory ex­ periments for reproducing the main aspects of astrophysical jets and compar­ ing them with observations. The discussion has been focused on the following topics: • Observations and intepretions of jets from young stars and AGNs, comparisons of models with observations; • MHO accelerations of jets: steady self-similar models, MHO numerical simula­ tions of time-dependent accelerations mechanisms; • Jet stability and interaction with the ambient: formation of knots in YSO jets, jet survival to instabilities, deceleration of relativistic jets in FRI sources, simulations of jets-IGM interactions, jets propagation and galaxy formation; • Numerical codes and their validation: relativistic MHO codes, comparisons among different numerical schemes, jets in the laboratory and code validation. These topics have been discussed intensively during the meeting, and the out­ come of these discussions is presented in this volume. The contributions have been divided in five sections