Relativistic flows in astrophysics
著者
書誌事項
Relativistic flows in astrophysics
（Lecture notes in physics, 589）（Physics and astronomy online library）
Springer, c2002
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注記
Includes bibliographical references and index
内容説明・目次
内容説明
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.
目次
Radiative Processes in Relativistic Outflows.- Particle Acceleration at Relativistic Shocks.- Jet Formation and Collimation.- The Evolution of Classical Double Radio Galaxies.- Blazars.- Relativistic Outflows from X-ray Binaries ('Microquasars').- Gamma-Ray Bursts: The Afterglow Revolution.- Observations and Simulations of Relativistic Jets.- 3D Relativistic Hydrodynamics.- Epilogue.
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