The correlation of narrow line emission and X-ray luminosity in active galactic nuclei
H. Netzer, V. Mainieri, P. Rosati, Benny Trakhtenbrot
Abstract
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H. Netzer, V. Mainieri, P. Rosati, Benny Trakhtenbrot
Abstract
Open-access reader
Aims.We combine emission line and X-ray luminosities for 45 sources from the Chandra Deep Field South (CDF-S), and seven HELLAS sources, to obtain a new sample of 52 X-ray selected type-II active galactic nuclei (AGNs). Eighteen of our sources are very luminous with a typical, absorption-corrected 2–10 keV luminosity of erg s-1 (type-II QSOs).
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Aims.We combine emission line and X-ray luminosities for 45 sources from the Chandra Deep Field South (CDF-S), and seven HELLAS sources, to obtain a new sample of 52 X-ray selected type-II active galactic nuclei (AGNs). Eighteen of our sources are very luminous with a typical, absorption-corrected 2–10 keV luminosity of erg s-1 (type-II QSOs).
Key concepts: QSOS, Active galactic nucleus, Physics, Astrophysics, Luminosity, X-ray, Line (geometry), Astronomy