The change from accretion via a thin disk to a coronal flow: Dependence on the viscosity of the hot gas

Astronomy and Astrophysics

Volumn 380, Issue 2, 2001, Pages 739-744

  Meyer Hofmeister, E ^a   Meyer, F ^a  

^a MAX PLANCK INSTITUT FÜR ASTROPHYSIK   (Germany)

Author keywords

Accretion disks; Black hole physics; Galaxies: nuclei; X rays: galaxies

Indexed keywords

EID: 0035578314     PISSN: 00046361     EISSN: None     Source Type: Journal    
DOI: 10.1051/0004-6361:20011449     Document Type: Article

References (29)