MARC Record from harvard_bibliographic_metadata

LEADER: 02668nam a22004575a 4500
001 013831142-0
005 20131206193858.0
008 121227s1997 gw | s ||0| 0|eng d
020 $a9783540687153
020 $a9783540687153
020 $a9783540628668
024 7 $a10.1007/BFb0105816$2doi
035 $a(Springer)9783540687153
040 $aSpringer
050 4 $aQB4
072 7 $aPG$2bicssc
072 7 $aSCI004000$2bisacsh
072 7 $aNAT033000$2bisacsh
082 04 $a520$223
100 1 $aMeyer-Hofmeister, Emmi,$eeditor.
245 10 $aAccretion Disks — New Aspects :$bProceedings of the EARA Workshop Held in Garching, Germany, 21–23 October 1996 /$cedited by Emmi Meyer-Hofmeister, Henk Spruit.
264 1 $aBerlin, Heidelberg :$bSpringer Berlin Heidelberg,$c1997.
300 $aXIII, 358 p.$bonline resource.
336 $atext$btxt$2rdacontent
337 $acomputer$bc$2rdamedia
338 $aonline resource$bcr$2rdacarrier
347 $atext file$bPDF$2rda
490 1 $aLecture Notes in Physics,$x0075-8450 ;$v487
505 0 $aFrom the contents: X-ray spectrum of low-mass X-ray binaries -- Black holes in X-ray binaries -- GX 339-4 -- BH and NS binaries -- Ion illumination -- Anisotropic illumination in Seyfert I galaxies -- Disk instabilities and binary evolution -- Dwarf nova outbursts -- Radiation transfer in disks of CVs -- Modelling magnetised accretion disks -- Causal viscosity -- Nonlinear evolution of a single mode -- The stability of magnetically threaded accretion disks -- Equilibrium and stability of an accretion disk containing a magnetic field -- Precessing disks.
520 $aThe most luminous compact objects are powered by accretion of mass. Accretion disks are the one common and fundamental element of these sources on widely different scales, ranging from close stellar binaries, galactic black holes and X-ray pulsars to active galactic nuclei (AGN). Key new developments in theory and observations, reviewed by experts in the field, are presented in this book. The contributions to the workshop cover the puzzles presented by the X-UV spectra of AGN and their variability, the recent numerical simulations of magnetic fields in disks, the remarkable behavior of the superluminal source 1915+105 and the "bursting pulsar" 1744-28, to mention a few of the topics.
650 20 $aAstrophysics.
650 20 $aAstronomy.
650 10 $aPhysics.
650 0 $aPhysics.
650 0 $aAstronomy.
650 0 $aAstrophysics.
700 1 $aSpruit, Henk,$eeditor.
776 08 $iPrinted edition:$z9783540628668
830 0 $aLecture Notes in Physics ;$v487.
988 $a20131114
906 $0VEN