252-alpha recombination-line emission from the direction of the galactic centre

Details 252-alpha recombination-line emission from the direction of the galactic centre 252-alpha recombination-line emission from the direction of the galactic centre

Feb 1977

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1977mnras.178p..37p&link_type=abstract

Monthly Notices of the Royal Astronomical Society, vol. 178, Feb. 1977, p. 37P-40P.

Astronomy and Astrophysics

Astronomy

1

Emission Spectra, Galactic Nuclei, Galactic Radio Waves, H Alpha Line, Radiative Recombination, Carbon, Continuous Radiation, Electron Transitions, H Beta Line, Line Spectra, Stimulated Emission

Scientific paper

Strong (greater than 1K) 252-alpha radio recombination lines of hydrogen
and carbon have been detected from the direction of the Galactic Center.
The intensity of the hydrogen 252-alpha line appears to be enhanced by
stimulated emission. An upper limit is put on the intensity of the
317-beta transition for hydrogen.

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