Virtual Astrophysical Jets: Theory Versus Observations
Editat de Silvano Massaglia, Gianluigi Bodo, P. Rossien Limba Engleză Paperback – 14 mar 2012
Preț: 621.74 lei
Preț vechi: 731.45 lei
-15% Nou
Puncte Express: 933
Preț estimativ în valută:
118.99€ • 125.17$ • 99.28£
118.99€ • 125.17$ • 99.28£
Carte tipărită la comandă
Livrare economică 09-23 ianuarie 25
Preluare comenzi: 021 569.72.76
Specificații
ISBN-13: 9789048158560
ISBN-10: 9048158567
Pagini: 288
Ilustrații: XV, 269 p. 85 illus.
Dimensiuni: 155 x 235 x 15 mm
Greutate: 0.41 kg
Ediția:2004
Editura: SPRINGER NETHERLANDS
Colecția Springer
Locul publicării:Dordrecht, Netherlands
ISBN-10: 9048158567
Pagini: 288
Ilustrații: XV, 269 p. 85 illus.
Dimensiuni: 155 x 235 x 15 mm
Greutate: 0.41 kg
Ediția:2004
Editura: SPRINGER NETHERLANDS
Colecția Springer
Locul publicării:Dordrecht, Netherlands
Public țintă
ResearchCuprins
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.
Caracteristici
Provides a global view on stellar jets and extragalactic jets unlike other books which deal with only one of these The authors are among the most active scientists in the field of theoretical interpretation of the astrophysical jets phenomenology and therefore this book can be considered as the most up-to-date in this field Astrophysical jets are collimated outflows of matter and fields that originate typically, but not uniquely, from Active Galactic Nuclei (AGNs) and young stars (YSOs). Jets from AGNs have linear sizes ranging from few up to thousand light years and velocities close to the speed of light, whereas jets from YSOs may reach few parsecs in size and some hundreds kilometers per second in speed. The study of astrophysical jets is utterly important since intimately connected with the formation and evolution of galaxies and stars and the dynamical processes of the interstellar and intergalactic medium