Observations of heavy element radio recombination lines from C II regions

Details Observations of heavy element radio recombination lines from C II regions Observations of heavy element radio recombination lines from C II regions

Mar 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984apj...278..604s&link_type=abstract

Astrophysical Journal, Part 1 (ISSN 0004-637X), vol. 278, March 15, 1984, p. 604-609. Research supported by the Perkin-Elmer Cor

Astronomy and Astrophysics

Astronomy

11

Abundance, Cosmochemistry, Heavy Elements, Hydrogen Clouds, Nebulae, Radio Sources (Astronomy), Carbon, Radiative Recombination, Sulfur

Scientific paper

The 166-alpha radio recombination lines of carbon and a heavier element identified as sulfur were observed from W48, S87, and S88B with the Arecibo 1000 foot (305 m) telescope. The C166-alpha line was observed from the C II region M78. Upper limits were set for the gaseous atomic abundances of silicon, magnesium, and iron from the absence of observable radio recombination lines. Lower limits were derived for gaseous atomic carbon.

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