The Jet Paradigm : From Microquasars to Quasars

These Lecture Notes focus on the physics of relativistic jet sources in the universe, from galactic microquasars to active galactic nuclei (AGN). The early 21st century is an epoch in which a large number of high-energy astronomical missions are underway (RossiXTE, Chandra, XMM-Newton, INTEGRAL, Swi...

Disgrifiad llawn

Wedi'i Gadw mewn:
Manylion Llyfryddiaeth
Prif Awdur: Belloni, Tomaso (Golygydd)
Fformat: Livre numérique
Iaith:Anglais
Cyhoeddwyd: Berlin, Heidelberg : Springer Berlin Heidelberg [20..].
Cham : Springer Nature
Rhifyn:1st ed. 2010.
Cyfres:Lecture Notes in Physics 794
Pynciau:
Mynediad Ar-lein:Accès sur la plateforme de l'éditeur
Accès sur la plateforme Istex
Accès Université d'Orléans
Accès INSA CVL
Nodyn: Archives Springer e-books (Licence nationale)
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Edition sous un autre format:• The jet paradigm, from microquasars to quasars, T. Belloni (ed.), Heidelberg, Springer Verlag, 2010, 1 vol. (XI-290 p.), The lecture notes in physics, 978-3-540-76936-1
• The Jet Paradigm, Texte imprimé, 9783540869641
• The Jet Paradigm, Texte imprimé, 9783642262159
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505 1 |a Microquasars: Summary and Outlook X-Ray Emission from Black-Hole Binaries States and Transitions in Black Hole Binaries Radio Emission and Jets from Microquasars #x2018;Disc#x2013;Jet#x2019; Coupling in Black Hole X-Ray Binaries and Active Galactic Nuclei From Multiwavelength to Mass Scaling: Accretion and Ejection in Microquasars and AGN Jets in Active Galactic Nuclei X-Ray Variability of AGN and Relationship to Galactic Black Hole Binary Systems Theory of Magnetically Powered Jets General Relativistic MHD Jets 
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520 |a These Lecture Notes focus on the physics of relativistic jet sources in the universe, from galactic microquasars to active galactic nuclei (AGN). The early 21st century is an epoch in which a large number of high-energy astronomical missions are underway (RossiXTE, Chandra, XMM-Newton, INTEGRAL, Swift, Suzaku). The wealth of X-ray and gamma-ray data, coupled with ground-based observations in the optical/IR/radio bands, provides an increasing amount of information on microquasars, allowing the investigation of the physical processes for the formation and the evolution of relativistic jets, as well as their relation to the accretion process. The information obtained from galactic relativistic jet systems is particularly important in that it can be compared with that from active galactic nuclei. The comparative study of these two classes of objects allows us to overcome their separate intrinsic limitations and is the only way to arrive at a comprehensive understanding of the accretion/ejection phenomenon. This book covers the topic of accretion/ejection in relativistic jet sources with a broad approach, from microquasars to AGN, discussing both observational and theoretical aspects. The aim is to present a broad view of the field and the current standpoint now that the first comparative studies have opened the way to a global study at a mass scale. Written in a pedagogical lecture notes style, the book benefits students and newcomers to jet astrophysics as well as lecturers and researchers 
650 |a Astrophysique 
650 |a Gravitation 
650 |a Noyaux actifs de galaxies 
650 |a Physique 
650 |a Quasars 
650 |a Microquasars 
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