The L-alpha/H-beta/P-alpha ratio in the quasar PG 0026+129

Details The L-alpha/H-beta/P-alpha ratio in the quasar PG 0026+129 The L-alpha/H-beta/P-alpha ratio in the quasar PG 0026+129

Dec 1978

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1978apj...226l..57b&link_type=abstract

Astrophysical Journal, Part 2 - Letters to the Editor, vol. 226, Dec. 1, 1978, p. L57-L59.

Astronomy and Astrophysics

Astronomy

17

H Lines, Line Spectra, Quasars, Ultraviolet Astronomy, H Beta Line, Lyman Spectra, Paschen Series, Satellite-Borne Instruments

Scientific paper

Observations of the quasar PG 0026+129 with the International Ultraviolet Explorer have determined its L-alpha intensity. In conjunction with visual and infrared observations by Puetter et al. (1978), a L-alpha/H-beta/P-alpha ratio of 6:1:1.4 is derived. The ratios differ from those found in 3C 273. The implications of these observations are discussed.

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