Contribution of the disk emission to the broad emission lines in AGNs: Two-component model

Astronomy and Astrophysics

Volumn 423, Issue 3, 2004, Pages 909-918

  Popovic L C ^a,b,c   Mediavilla, E ^d   Bon, E ^a,c   Ilic D ^e  

^a ASTRONOMICAL OBSERVATORY   (Serbia)

^b ASTROPHYSIKALISCHES INSTITUT POTSDAM   (Germany)

^c ISAAC NEWTON INSTITUTE OF CHILE   (Chile)

^d INSTITUTO DE ASTROFÍSICA DE CANARIAS   (Spain)

^e UNIVERSITY OF BELGRADE   (Serbia)

Author keywords

Accretion, accretion disks; Galaxies: Seyfert; Line: profiles

Indexed keywords

COMPUTER SOFTWARE; MATHEMATICAL MODELS; SHOCK WAVES; SIGNAL TO NOISE RATIO; SPECTRUM ANALYSIS; X RAY ANALYSIS;

ACCRETION; ACCRETION DISKS; GALAXIES:SEYFERT; LINE:PROFILES;

GALAXIES;

EID: 4344591789     PISSN: 00046361     EISSN: None     Source Type: Journal    
DOI: 10.1051/0004-6361:20034431     Document Type: Article

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