JET Simulations, Experiments, and Theory Ten Years After JETSET. What Is Next? /

• Συγγραφή απο Οργανισμό/Αρχή: SpringerLink (Online service)
• Άλλοι συγγραφείς: Sauty, Christophe (Επιμελητής έκδοσης, http://id.loc.gov/vocabulary/relators/edt)
• Μορφή: Ηλεκτρονική πηγή Ηλ. βιβλίο
• Γλώσσα: English
• Έκδοση: Cham : Springer International Publishing : Imprint: Springer, 2019.
• Έκδοση: 1st ed. 2019.
• Σειρά: Astrophysics and Space Science Proceedings, 55
• Θέματα: Astrophysics.; Observations, Astronomical.; Astronomy-Observations.; Physics.; Astrophysics and Astroparticles.; Astronomy, Observations and Techniques.; Numerical and Computational Physics, Simulation.

 In 2008, the European FP6 JETSET project ended. JETSET, for Jet, Simulations, Experiments, and Theory, was a joint research network of European expert teams on protostellar jets. The present proceedings are a collection of contributions presenting new results obtained by those groups since the end of the JETSET program. This is also the occasion to celebrate Kanaris Tsinganos' important contributions to this network and for his enlightening insight in the subject that inspired us all. Some of the former JETSET students are now in the academic world and the subject has never been so alive. So we present here a collection of results of what has been done in the field of protostellar jets in the past ten years from the theoretical, numerical, observational and experimental point of view. We also present new challenges in the field of protostellar jets and what we should expect from the development of new instruments and new numerical codes in the near future. We also gather results on the impact of the study of protostellar jets on other jet studies in particular on relativistic jets. As a matter of fact, it is time for a new network. 

 Part I -- Theory and Models -- Magnetorotational Turbulence, Dynamo Action and Transport in Convective Disks -- An Energetic Criterion for Astrophysical Winds and Jets -- Meridional Self-Similar MHD Relativistic Flows Around Kerr Black Holes -- Part II -- Simulations -- Modelling the Accretion on Young Stars, Recent Results and Perspectives -- Radiation Magnetohydrodynamic Models and Spectral Signatures of Plasma Flows Accreting onto Classical T Tauri Stars -- Mass Accretion Impacts in Classical T Tauri Stars: A Multi-Disciplinary approach -- High Energy Emission from Shocks Due to Jets and Accretion in Young Stars with Disks: Combining Observations, Numerical Models, and Laboratory Experiments -- On the Origin of the X-ray Emission in Protostellar Jets Close to the Launching Site -- Simulating Accretion and Outflow Regions in YSOs -- Modeling Jet Launching from Accretion Disks -- Relativistic 3D Hydrodynamic Simulations of the W50-SS433 System -- Knots in Relativistic Transverse Stratified Jets -- Part III -- Observations and Experiments -- ALMA Polarimetric Studies of Rotating Jet/Disk Systems -- Analysis of the Physical Properties of Jets/Outflows in T Tauri Stars -- X-Shooter Survey of Jets and Winds in T Tauri Stars -- Accretion Bursts from Young Stars -- The Musca Molecular Cloud: An Interstellar Symphony -- Laboratory Astrophysics at Extreme Light Infrastructure - Nuclear Physics -- Part IV -- Future Projects -- GIARPS/GRAVITY Survey: Broad-band 0.44-2.4 Micron High-Resolution Spectra of T-Tauri and Herbig AeBe Stars. Combining High Spatial and High Spectral Resolution Data to Unveil the Inner Disc Physics -- Observational Constraints on the Conservation of Momentum and Energy in Jet-driven Molecular Outflows -- Part V -- A Tribute to K. Tsinganos -- A Short Tribute to Kanaris Tsinganos, Conclusions to This Book.