Detection of radio recombination lines in the Seyfert galaxy MRK 668

Details Detection of radio recombination lines in the Seyfert galaxy MRK 668 Detection of radio recombination lines in the Seyfert galaxy MRK 668

Jun 1980

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1980apj...238..818b&link_type=abstract

Astrophysical Journal, Part 1, vol. 238, June 15, 1980, p. 818-822.

Astronomy and Astrophysics

Astrophysics

18

Alpha Particles, Ion Recombination, Line Spectra, Radio Spectra, Seyfert Galaxies, Astronomical Models, Emission Spectra, Galactic Nuclei, Ionized Gases, Stimulated Emission

Scientific paper

The detection of H83-alpha and H99-alpha radio recombination lines in
the Markarian-Seyfert galaxy Mrk 668 (=OQ 208) is reported. The emission
mechanism for these lines is stimulated emission in the nuclear ionized
gas by the compact nonthermal source in the nucleus. A simple model for
this region which accounts for the radio lines is presented.

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