Please use this identifier to cite or link to this item: https://research.matf.bg.ac.rs/handle/123456789/3074
Title: Two-component model for III Zw 2 broad line region
Authors: Bon, E
Stanić, N
Ilić, Dragana 
Kubicela, A
Mediavilla, E G
Popović, Luka 
Affiliations: Astronomy 
Astronomy 
Issue Date: 2003
Rank: M63
Publisher: Beograd : Astronomska opservatorija
Related Publication(s): IV Serbian Conference on Spectral Line Shapes
Journal: Publications of the Astronomical Observatory of Belgrade)
Conference: Serbian Conference on Spectral Line Shapes (4 ; 2003 ; Aranđelovac)
Abstract: 
We have modelled the central emitting broad line region (BLR) of the III Zw2 using the Hα Hβ Lyα and Mg II (2798) broad lines. We proposed that two-component model, consisting of inner Keplerian relativistic disk and an outer emitting structure that surrounds the disk, can explain the shape of III Zw 2 Broad Lines
URI: https://research.matf.bg.ac.rs/handle/123456789/3074
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