The Shape of III Zw2 Hα Line: Evidence of Keplerian Relativistic Disk

Bon, E.; Popović, L. Č; Mediavilla, E.
Referencia bibliográfica

Astronomische Gesellschaft Abstract Series, Vol. 18. Abstracts of Contributed Talks and Posters presented at the Annual Scientific Meeting of the Astronomische Gesellschaft at the Joint European and National Meeting JENAM 2001 of the European Astronomical Society and the Astronomische Gesellschaft at Munich, September 10-15, 2001, abstract #P175.

Fecha de publicación:
0
2001
Número de autores
3
Número de autores del IAC
0
Número de citas
0
Número de citas referidas
0
Descripción
We have analyzed the shape of III Zw2 Hα emission line observed at Isaac Newton telescope. A model with a Keplerian relativistic disk plus one emission region more very well fit the line profile. Disk emission contribute the line wings, while the line core is probably originated in a region which surrounds the disk.