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

Bibcode
2001AGM....18.P175B
Bon, E.; Popović, L. Č; Mediavilla, E.
Bibliographical reference

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.

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0
2001
Number of authors
3
IAC number of authors
0
Citations
0
Refereed citations
0
Description
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.
Type
Non-refereed

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