Two-component model for III Zw 2 broad line region

Details Two-component model for III Zw 2 broad line region Two-component model for III Zw 2 broad line region

Oct 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003pobeo..76..171b&link_type=abstract

Publications of the Astronomical Observatory of Belgrade (ISSN 0373-3742), No. 76, p. 171 - 174 (2003). In: IV Serbian Conferenc

Astronomy and Astrophysics

Astronomy

Active Galaxies, Broad-Line Regions

Scientific paper

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.

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