X-ray and optical continua of active galactic nuclei with extreme Fe II emission | Zendy

A. Lawrence | Zendy; Martin Elvis | Zendy; B. J. Wilkes | Zendy; I. M. McHardy | Zendy; N. Brandt | Zendy

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X-ray and optical continua of active galactic nuclei with extreme Fe II emission

Author(s) -

A. Lawrence,

Martin Elvis,

B. J. Wilkes,

I. M. McHardy,

N. Brandt

Publication year - 1997

Publication title -

monthly notices of the royal astronomical society

Language(s) - English

Resource type - Journals

SCImago Journal Rank - 2.058

H-Index - 383

eISSN - 1365-8711

pISSN - 0035-8711

DOI - 10.1093/mnras/285.4.879

Subject(s) - physics , astrophysics , active galactic nucleus , rosat , spectral line , balmer series , quasar , luminosity , spectral index , emission spectrum , x ray , galaxy , line (geometry) , astronomy , optics , geometry , mathematics

We present the results of ROSAT PSPC observations of three active galactic nuclei (AGN) with extremely strong Fe II emission (PHL 1092, IRAS 07598 + 6508 and I Zw 1) and two AGN with very weak Fe II emission (Mrk 10 and 110). The weak Fe II emitters have X-ray spectra typical of Type 1 AGN (α = 1.35 and 1.41, where α is the spectral energy index). Of the strong Fe II emitters, two have steep spect...

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