The thermal-viscous disk instability model in the AGN context

Astronomy and Astrophysics

Volumn 496, Issue 2, 2009, Pages 413-421

  Hameury, J M ^a   Viallet, M ^a   Lasota, J P ^b,c  

^a OBSERVATOIRE DE STRASBOURG   (France)

^b INSTITUT D'ASTROPHYSIQUE DE PARIS   (France)

^c JAGIELLONIAN UNIVERSITY   (Poland)

Author keywords

Accretion, accretion disks; Galaxies: active; Instabilities; Stars: dwarf novae

Indexed keywords

COOLING; DISKS (MACHINE COMPONENTS); GALAXIES; HEATING; IRRADIATION; MACH NUMBER; STABILITY; STARS;

ACCRETION DISKS; ACCRETION RATES; ACCRETION, ACCRETION DISKS; BLACK HOLES; CATACLYSMIC VARIABLES; DWARF NOVAE; GALAXIES: ACTIVE; INSTABILITIES; INSTABILITY MODELS; LONG-TERM VARIABILITIES; LOW-MASS X-RAY BINARIES; NUMERICAL CODES; QUIESCENT STATE; RADIAL STRUCTURES; SMALL VARIATIONS; SOFT X-RAYS; STARS: DWARF NOVAE; TIME-SCALES; VERY LOW MASS; X-RAY SOURCES;

DISKS (STRUCTURAL COMPONENTS);

EID: 62749168364     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361/200810928     Document Type: Article

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