The advection-dominated accretion flow+thin accretion disk model for two low-luminosity active galactic nuclei: M81 and NGC 4579

Research in Astronomy and Astrophysics

Volumn 9, Issue 4, 2009, Pages 401-408

  Xu, Ya Di ^a   Cao, Xin Wu ^b  

^a SHANGHAI JIAO TONG UNIVERSITY   (China)

^b CHINESE ACADEMY OF SCIENCES   (China)

Author keywords

Accretion, accretion disks; Black hole physics; Galaxies: individual (M81, NGC 4579); Galaxies:active; Radiation mechanisms: thermal

Indexed keywords

EID: 68849116479     PISSN: 16744527     EISSN: None     Source Type: Journal    
DOI: 10.1088/1674-4527/9/4/003     Document Type: Article

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