On the nature of the extragalactic radio recombination lines

Details On the nature of the extragalactic radio recombination lines On the nature of the extragalactic radio recombination lines

Mar 1978

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1978a%26a....64....1s&link_type=abstract

Astronomy and Astrophysics, vol. 64, no. 1-2, Mar. 1978, p. 1-8. Research supported by the Nederlandse Organisatie voor Zuiver-

Astronomy and Astrophysics

Astronomy

16

Extragalactic Radio Sources, Hydrogen Recombinations, Line Spectra, Radio Astronomy, Stimulated Emission, Astronomical Models, H Alpha Line, Nonthermal Radiation, Radio Spectroscopy, Spectrum Analysis, Spontaneous Emission

Scientific paper

Observations of the H 166-alpha, H 110-alpha, and H 76-alpha
recombination lines from M82 are used to show that the observed line
emission is predominantly stimulated. It is argued that the recently
detected H102-alpha line from NGC 253 may also be due primarily to
stimulation by nonthermal background radiation.

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