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Titlebook: Relativistic Flows in Astrophysics; Axel W. Guthmann,Markos Georganopoulos,Alexandre M Book 2002 Springer-Verlag Berlin Heidelberg 2002 ac

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書目名稱Relativistic Flows in Astrophysics
編輯Axel W. Guthmann,Markos Georganopoulos,Alexandre M
視頻videohttp://file.papertrans.cn/827/826214/826214.mp4
概述Bridges the gap between standard textbook material and the research level.Includes supplementary material:
叢書名稱Lecture Notes in Physics
圖書封面Titlebook: Relativistic Flows in Astrophysics;  Axel W. Guthmann,Markos Georganopoulos,Alexandre M Book 2002 Springer-Verlag Berlin Heidelberg 2002 ac
描述1. 1 Schematic Picture of AGN Some galaxies are known to emit radiation with extremely high luminosities from a rather small volume in the ??ray, X-ray and UV continuum. Such active cores are the so-called Active Galactic Nuclei (AGN) and the radiation is commonly believed to be a result of gravitational energy released by matter spiraling around 9 a supermassive central black hole of about 10 M (see Fig. 1).Though the central engine which produces the enormous observed activity cannot be resolved observationally, a standard picture of an AGN has gradually emerged to explain the richness of the radiation spectra: ? an accretion disk with radius from about 2 to 100 gravitational radii, R , g feeding the central black hole and emitting mainly in the UV and soft X-rays; ? the broad line optically emitting clouds (BLR), which seem to be absent in 3 some sources (e. g. FRI, see hereafter) and extend up to a few 10 R from g the center.
出版日期Book 2002
關(guān)鍵詞active galactic nuclei; astrophysical jets; astrophysics; gamma-ray bursts; particle acceleration; relati
版次1
doihttps://doi.org/10.1007/3-540-46025-X
isbn_softcover978-3-642-07804-0
isbn_ebook978-3-540-46025-1Series ISSN 0075-8450 Series E-ISSN 1616-6361
issn_series 0075-8450
copyrightSpringer-Verlag Berlin Heidelberg 2002
The information of publication is updating

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Blazars,ration, time and energy transformations. This definition of blazars broadly includes BL Lac objects (BL Lac) and Flat Spectrum Radio Quasars (FSRQ), where the former ones are typically featureless while large and intense line emission is detectable in the optical-UV spectrum of quasars.
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,Relativistic Outflows from X-ray Binaries (‘Microquasars’),esence of radio emission, and the related anti-correlation between jet strength and mass-accretion rate as inferred from X-ray studies alone. I briefly discuss possible future directions for research and compare X-ray binary jets to those from Active Galactic Nuclei and Gamma Ray Bursts.
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Observations and Simulations of Relativistic Jets, of the non—thermal emission from these hydrodynamical models, and its comparison with actual sources, is proving as one of the most powerful tools in the understanding of the physical processes taking place in these jets. This paper reviews some of the recent observational results, as well as the numerical models used to interpret them.
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Particle Acceleration at Relativistic Shocks, the nonrelativistic Fermi mechanism and the differences introduced by relativistic flows. I present numerical calculations of the accelerated particle spectrum, and examine the maximum energy attainable by this process. I briefly consider the minimum energy for Fermi acceleration, and a possible el
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