The accretion mechanism in low-power radio galaxies

Astronomy and Astrophysics

Volumn 486, Issue 1, 2008, Pages 119-130

  Balmaverde, B ^a   Baldi, R D ^b   Capetti, A ^a  

^a OSSERVATORIO ASTRONOMICO DI TORINO   (Italy)

^b UNIVERSITY OF TURIN   (Italy)

Author keywords

Galaxies: active; Galaxies: elliptical and lenticular, cD; Galaxies: ISM; Galaxies: jets

Indexed keywords

DISKS (STRUCTURAL COMPONENTS); ESTIMATION; JETS; LUMINANCE; MECHANISMS; MOLECULAR INTERACTIONS; OPTICAL PROPERTIES; STANDARDS;

(E ,3E) PROCESS; (PL) PROPERTIES; ACCRETION DISKS; ACCRETION RATES; CHANDRA; GLOBAL CHANGES; HOT GASSES; JET POWER; LINEAR RELATIONS; LOW POWERS; MASS FLOWS; NUCLEAR ACTIVITIES; ORDERS-OF-MAGNITUDE; RADIATIVE EFFICIENCY; RADIO GALAXIES; REST MASS; SPHERICAL(PIVOT); SURFACE BRIGHTNESSES; TEMPERATURE PROFILING; X-RAY EMISSIONS;

GALAXIES;

EID: 46649110974     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361:200809810     Document Type: Article

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