Prospects for observing low-frequency radio recombination lines toward quasars

Details Prospects for observing low-frequency radio recombination lines toward quasars Prospects for observing low-frequency radio recombination lines toward quasars

Feb 1983

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983azh....60...29v&link_type=abstract

(Astronomicheskii Zhurnal, vol. 60, Jan.-Feb. 1983, p. 29-33) Soviet Astronomy (ISSN 0038-5301), vol. 27, Jan.-Feb. 1983, p. 18-

Astronomy and Astrophysics

Astronomy

Line Spectra, Quasars, Radiative Recombination, Radio Sources (Astronomy), Radio Spectra, Absorption Spectra, Heavy Elements, Photoabsorption, Radiant Flux Density

Scientific paper

The possibility is evaluated of observing low-frequency radio recombination lines of heavy elements in the direction toward a quasar when intervening regions responsible for optical absorption lines are present. The physical parameters of the absorption zones imply that the dielectronic-recombination mechanism should be taken into account, much enhancing the lines of heavy elements compared with the hydrogen lines.

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