LEADER 05407nam 2200697Ia 450 001 9910141156603321 005 20210104163331.0 010 $a3-527-64175-0 010 $a1-283-37952-X 010 $a9786613379528 010 $a3-527-64176-9 035 $a(CKB)2670000000138715 035 $a(EBL)827182 035 $a(OCoLC)769343050 035 $a(SSID)ssj0000640505 035 $a(PQKBManifestationID)11377914 035 $a(PQKBTitleCode)TC0000640505 035 $a(PQKBWorkID)10612926 035 $a(PQKB)10451224 035 $a(MiAaPQ)EBC827182 035 $a(EXLCZ)992670000000138715 100 $a20111229d2012 uy 0 101 0 $aeng 135 $aur|n|---||||| 181 $ctxt 182 $cc 183 $acr 200 10$aRelativistic jets from active galactic nuclei$b[electronic resource] /$fedited by Markus Bo?ttcher, Daniel E. Harris, and Henric Krawczynski 210 $aWeinheim $cWiley-VCH$d2012 215 $a1 online resource (424 p.) 300 $aDescription based upon print version of record. 311 $a3-527-64174-2 311 $a3-527-41037-6 327 $aRelativistic Jets from Active Galactic Nuclei; Contents; Preface; List of Contributors; Glossary and Acronyms; Part One Introduction; 1 Introduction and Historical Perspective; 1.1 A Brief History of Jets; 1.1.1 Synchrotron Emission as the Primary Process for Continuum Radio Sources; 1.1.2 Occurrence/Ubiquity of Radio Jets; 1.1.3 Origin of the Notion that SMBHs Reside in All Galactic Nuclei; 1.1.4 Working Out of Relativistic Effects; 1.1.5 Microquasars; 1.2 Jets at Optical, UV, X-Rays and -Rays; 1.2.1 HST Optical/UV Jets; 1.2.2 X-Ray Jets; 1.2.3 Jets in -Rays; 1.2.4 Gamma-Ray Bursts 327 $a1.3 The Role of Simulations1.4 Jet Composition; 1.4.1 Options; 1.4.2 Constraints; 1.5 Some Things (We Think) We Know, and Some (We Know) We Don't; References; Part Two Theory Basics; 2 Special Relativity of Jets; 2.1 Space-Time, Four-Vectors, and Lorentz Invariance; 2.1.1 Interaction Thresholds; 2.2 Lorentz Transformations; 2.3 Relativistic Jet Diagnostics; 2.3.1 Size Constraint from Variability; 2.3.2 Superluminal Motion; 2.3.3 Lorentz Factor and Viewing Angle Estimates; References; 3 Radiation Processes; 3.1 Radiative Transfer: Definitions; 3.1.1 Radiative Flux, Intensity, Energy Density 327 $a3.1.2 The Radiative Transfer Equation3.2 Nonthermal Emission Processes; 3.2.1 Synchrotron Radiation; 3.2.2 Compton Scattering; 3.2.3 Absorption and Pair Production; 3.2.4 -Hadron Interactions; 3.3 Electromagnetic Cascades; References; 4 Central Engines: Acceleration, Collimation and Confinement of Jets; 4.1 Central Engine; 4.1.1 Bondi Flow; 4.1.2 Disk Accretion; 4.1.3 The Eddington Limit; 4.1.4 Fuel Supply; 4.2 Magnetic Fields; 4.2.1 Basics; 4.2.2 Powering Magnetic Winds and Jets; 4.2.3 The Blandford-Znajek Mechanism; 4.3 Confinement, Collimation, and Acceleration of Jets 327 $a4.3.1 Acceleration in Supersonic Regime4.3.2 Acceleration and Differential Collimation; 4.3.3 Jets and Magnetic Towers; References; Part Three Phenomenology; 5 Observational Details: Radio; 5.1 Overall Structures of Radio Sources; 5.1.1 Terminology; 5.2 Parsec-Scale Jets; 5.2.1 One-Sided Jets; 5.2.2 Two-Sided Jets; 5.2.3 VLBI Surveys; 5.2.4 Motions in the Jet; 5.2.5 Relativistic Beams; 5.2.6 Statistical Studies of Compact Jets with VLBI; 5.2.7 Spine-Sheath Configuration; 5.3 Kiloparsec-Scale Jets; 5.3.1 Correlations with Extended Structure and Luminosity; 5.3.2 The Two Jet "Flavors" 327 $a5.3.3 Internal Structures of Kiloparsec-Scale Radio Jets5.3.4 Jet Bending on Kiloparsec Scales; 5.4 Modeling Jet Kinematics from Radio Data; 5.4.1 Intensity Asymmetry Modeling: Velocity-Angle Degeneracy; 5.4.2 Polarization Asymmetry Modeling: Resolving the Degeneracy; 5.4.3 Velocity Fields in Weak-Flavor Jets; 5.4.4 Magnetic Field Evolution in Weak-Flavor Jets; 5.4.5 Emissivity Evolution in Weak-Flavor Jets; 5.4.6 Mass, Momentum and Energy Fluxes; 5.4.7 Comparisons with Strong-Flavor Jets; 5.5 Backflow in Bilobed FRI Sources?; References; 6 Optical, Infrared and UV Observations 327 $a6.1 A Historical Perspective 330 $aWritten by a carefully selected consortium of researchers working in the field, this book fills the gap for an up-to-date summary of the observational and theoretical status. As such, this monograph includes all used wavelengths, from radio to gamma, the FERMI telescope, a history and theory refresher, and jets from gamma ray bursts.For astronomers, nuclear physicists, and plasmaphysicists. 606 $aGalactic nuclei$vCongresses 606 $aGalaxies$xEvolution$xMathematical models$vCongresses 606 $aGalaxies$xFormation$xMathematical models$vCongresses 606 $aGalaxies$xFormation 608 $aElectronic books. 615 0$aGalactic nuclei 615 0$aGalaxies$xEvolution$xMathematical models 615 0$aGalaxies$xFormation$xMathematical models 615 0$aGalaxies$xFormation. 676 $a523.112 676 $a523.8 700 $aKrawczynski$b Henric$0968932 701 $aBo?ttcher$b Markus$0968933 701 $aHarris$b Daniel E$0860906 801 0$bMiAaPQ 801 1$bMiAaPQ 801 2$bMiAaPQ 906 $aBOOK 912 $a9910141156603321 996 $aRelativistic jets from active galactic nuclei$92201331 997 $aUNINA LEADER 03141nam 22007095 450 001 996641272003316 005 20250806175800.0 010 $a9783031827006 010 $a3031827007 024 7 $a10.1007/978-3-031-82700-6 035 $a(MiAaPQ)EBC31887313 035 $a(Au-PeEL)EBL31887313 035 $a(CKB)37345589200041 035 $a(DE-He213)978-3-031-82700-6 035 $a(OCoLC)1498688182 035 $a(EXLCZ)9937345589200041 100 $a20250123d2025 u| 0 101 0 $aeng 135 $aurcnu|||||||| 181 $ctxt$2rdacontent 182 $cc$2rdamedia 183 $acr$2rdacarrier 200 10$aVerification, Model Checking, and Abstract Interpretation $e26th International Conference, VMCAI 2025, Denver, CO, USA, January 20?21, 2025, Proceedings, Part I /$fedited by Krishna Shankaranarayanan, Sriram Sankaranarayanan, Ashutosh Trivedi 205 $a1st ed. 2025. 210 1$aCham :$cSpringer Nature Switzerland :$cImprint: Springer,$d2025. 215 $a1 online resource (428 pages) 225 1 $aLecture Notes in Computer Science,$x1611-3349 ;$v15529 311 08$a9783031826993 311 08$a303182699X 330 $aThe two-volume set LNCS 15529 and 15530 constitutes the proceedings of the 26th International Conference on Verification, Model Checking, and Abstract Interpretation, VMCAI 2025, held in Denver, CO, USA, during January 20?21, 2025. The 20 full papers together with 2 accepted tool papers and 18 full length regular and case-study papers presented in the proceedings were carefully reviewed and selected from 48 submissions. 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