04710nam 22006255 450 99646670240331620200701161606.03-540-46448-410.1007/3-540-54789-4(CKB)1000000000233731(SSID)ssj0000326214(PQKBManifestationID)12082544(PQKBTitleCode)TC0000326214(PQKBWorkID)10265090(PQKB)10458569(DE-He213)978-3-540-46448-8(PPN)155224158(EXLCZ)99100000000023373120121227d1991 u| 0engurnn|008mamaatxtccrRelativistic Hadrons in Cosmic Compact Objects[electronic resource] Proceedings of a Workshop Held in Koninki/Suhora, Poland 9–11 October 1990 /edited by Andrzej A. Zdziarski, Marek Sikora1st ed. 1991.Berlin, Heidelberg :Springer Berlin Heidelberg :Imprint: Springer,1991.1 online resource (XII, 183 p. 9 illus.) Lecture Notes in Physics,0075-8450 ;391Bibliographic Level Mode of Issuance: Monograph3-540-54789-4 Relativistic hadrons near accreting compact objects: Dynamical and radiative signatures -- Can ultrarelativistic neutrons from the central engine drive the outflow in broad absorption line QSOS? -- Inflation of stars by TeV neutrinos -- Electron-positron pair production in compact sources with energetic protons -- Limit cycles in electromagnetic cascades in compact objects -- Nuclear interactions near accreting black holes -- A new approach to hot accretion disks -- X-ray continuum emission caused by relativistic protons -- Pair cascade model constraints on energetic particle emission from active galactic nuclei -- Jets and hotspots in extragalactic radio sources -- Pion production in strong magnetic fields: A model for gamma-ray emission from accreting X-ray pulsars -- Particle acceleration at shock fronts in AGNs and jets -- Fermi particle acceleration in relativistic shocks: Preliminary nonlinear results -- Cosmic ray transport in AGNs and jets -- Particle Acceleration in Relativistic Shock waves with Oblique Magnetic Fields in the presence of Finite Amplitude Field perturbations -- Collisional Acceleration of Electrons in Central Regions of Active Galactic Nuclei -- Influence of Second-Order Fermi acceleration and Relativistic Shock Waves on Nonthermal Continuum Emission in Hot Spots -- Collimated Relativistic Winds Driven by Electromagnetic Forces -- Ultra-relativistic pulsar wind -- A model of pulsed gamma-radiation from the X-ray binary Hercules X-1/HZ Herculis -- Gamma-ray astronomy above 100 GeV -- High energy and very high energy gamma-rays from electromagnetic cascade induced by relativistic neutrons in AGN -- Near simultaneous optical and TeV observations of AE Aquarii.The articles in this book deal with energetic hadron processes near astrophysical compact objects, including compact binary systems and active galactic nuclei. A variety of observational results suggest that relativistic hadrons can be produced in the vicinity of these objects. Amongthe topics treated in detail are the question whether a large fraction of the energy produced by active galactic nuclei is channeled into a population of relativistic protons and the problem of the origin of very high and ultra-high energy gamma rays from galactic compact sources.Lecture Notes in Physics,0075-8450 ;391Observations, AstronomicalAstronomy—ObservationsAstrophysicsGeophysicsAstronomy, Observations and Techniqueshttps://scigraph.springernature.com/ontologies/product-market-codes/P22014Astrophysics and Astroparticleshttps://scigraph.springernature.com/ontologies/product-market-codes/P22022Geophysics/Geodesyhttps://scigraph.springernature.com/ontologies/product-market-codes/G18009Observations, Astronomical.Astronomy—Observations.Astrophysics.Geophysics.Astronomy, Observations and Techniques.Astrophysics and Astroparticles.Geophysics/Geodesy.523.01/97216Zdziarski Andrzej Aedthttp://id.loc.gov/vocabulary/relators/edtSikora Marekedthttp://id.loc.gov/vocabulary/relators/edtBOOK996466702403316Relativistic Hadrons in Cosmic Compact Objects2506281UNISA