Extreme Fe II emission from an IRAS quasar

Details Extreme Fe II emission from an IRAS quasar Extreme Fe II emission from an IRAS quasar

Nov 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988mnras.235..261l&link_type=abstract

Monthly Notices of the Royal Astronomical Society (ISSN 0035-8711), vol. 235, Nov. 1, 1988, p. 261-268.

Astronomy and Astrophysics

Astronomy

37

Emission Spectra, Infrared Astronomy Satellite, Quasars, Iron, Photoionization, X Ray Astronomy

Scientific paper

During an all-sky redshift survey of IRAS galaxies, the authors have discovered a very unusual quasar (IRAS source 07598+6508). The optical spectrum is dominated by extremely strong Fe II emission, roughly an order of magnitude stronger than that seen in so-called strong Fe II emitters. There seems to exist a very small class of super-strong Fe II emitters. Current photo-ionization models do not readily account for the extreme properties of these objects.

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