Two-component model for III Zw 2 broad line region

Bibcode
2003POBeo..76..171B
Bon, E.; Stanić, N.; Ilić, D.; Kubicela, A.; Mediavilla, E.; Popović, L. C.
Referencia bibliográfica

Publications of the Astronomical Observatory of Belgrade (ISSN 0373-3742), No. 76, p. 171 - 174 (2003). In: IV Serbian Conference on Spectral Line Shapes, Arandelovac, Serbia, 10-15 October 2003.

Fecha de publicación:
10
2003
Número de autores
6
Número de autores del IAC
0
Número de citas
0
Número de citas referidas
0
Descripción
We have modelled the central emitting broad line region (BLR) of the III Zw 2 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.
Tipo
Sin árbitro
Galaxias activas

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