A search for meter-wavelength hydrogen recombination lines, and constraints on the parameters of the ionized interstellar gas

Details A search for meter-wavelength hydrogen recombination lines, and constraints on the parameters of the ionized interstellar gas A search for meter-wavelength hydrogen recombination lines, and constraints on the parameters of the ionized interstellar gas

Feb 1982

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982azh....59...38a&link_type=abstract

(Astronomicheskii Zhurnal, vol. 59, Jan.-Feb. 1982, p. 38-43.) Soviet Astronomy, vol. 26, Jan.-Feb. 1982, p. 23-26. Translation

Astronomy and Astrophysics

Astronomy

2

H Lines, Hydrogen Ions, Hydrogen Recombinations, Interstellar Gas, Radio Sources (Astronomy), Very High Frequencies, Astronomical Spectroscopy, Constraints, Data Acquisition, Hydrogen Clouds, Ionized Gases, Radio Astronomy, Radio Spectra

Scientific paper

A search has been made for the H392 alpha-H394 alpha radio recombination
lines in the direction toward the sources Sgr A, M17, and W51. Upper
limits are set on the line/continuum intensity ratio: 0.0004 for Sgr A
and M17, and 0.0014 for W51. The parameters of the ionized interstellar
gas toward the three sources are estimated.

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