Decameter-wavelength carbon recombination lines toward Cassiopeia A

Details Decameter-wavelength carbon recombination lines toward Cassiopeia A Decameter-wavelength carbon recombination lines toward Cassiopeia A

Dec 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984pazh...10..846k&link_type=abstract

(Pis'ma v Astronomicheskii Zhurnal, vol. 10, Nov. 1984, p. 846-853) Soviet Astronomy Letters (ISSN 0360-0327), vol. 10, Nov.-Dec

Astronomy and Astrophysics

Astronomy

17

Astronomical Spectroscopy, Carbon, Line Spectra, Radio Sources (Astronomy), Absorption Spectra, Decametric Waves, Radiative Recombination, Resonance Lines

Scientific paper

A number of carbon recombination lines are detected in the 16.7 - 30 MHz range toward Cassiopeia A. Principal parameters of the C603α - C732α lines are measured. Physical conditions are analyzed of the region where observed absorption lines have been formed. The low-temperature dielectronic recombination mechanism is shown to be needed to explain the observational data.

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