Further evidence for the accretion disc origination of the double-peaked broad Hα of 3C 390.3
Author:
Publisher
Oxford University Press (OUP)
Subject
Space and Planetary Science,Astronomy and Astrophysics
Link
http://academic.oup.com/mnrasl/article-pdf/431/1/L112/4213316/slt019.pdf
Reference51 articles.
1. Massive black hole binaries in active galactic nuclei
2. Reverberation mapping of the emission line regions of Seyfert galaxies and quasars
3. A candidate sub-parsec supermassive binary black hole system
4. C 390.3, an N System with Two Emission Redshifts
5. Structure of line-emitting accretion disks in active galactic nuclei - ARP 102B
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2. Dependence of Narrow-line Region Sizes on [O iii] Luminosity in Low-redshift Active Galactic Nuclei with Double-peaked Broad Balmer Emission Lines;The Astrophysical Journal Supplement Series;2022-06-01
3. SDSS J154751.94+025550 with double-peaked broad H β but single-peaked broad H α: a candidate for central binary black hole system?;Monthly Notices of the Royal Astronomical Society;2021-08-28
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5. THE COMPLEX CIRCUMNUCLEAR ENVIRONMENT OF THE BROAD-LINE RADIO GALAXY 3C 390.3 REVEALED BYCHANDRAHETG;The Astrophysical Journal;2016-10-17
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