Infrared Spectroscopy of High-Redshift Quasars

Details Infrared Spectroscopy of High-Redshift Quasars Infrared Spectroscopy of High-Redshift Quasars

Oct 1994

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1994mnras.270..575b&link_type=abstract

Monthly Notices of the Royal Astronomical Society, Vol. 270, NO. 3/OCT1, P. 575, 1994

Astronomy and Astrophysics

Astronomy

20

Scientific paper

We present H and K spectra (showing redshifted Hα, Hβ and [O III] emission lines) of three radio-loud and three radio-quiet quasars with redshifts z >~ 2, which were obtained using CGS4 on UKIRT The [O III] λλ 4959 + 5007 lines are too weak to allow accurate determination of the redshift of the forbidden lines. The observed Balmer decrements are consistent with enhancement of Hα due to collisional excitation.

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