Radio recombination lines from carbon and heavier elements from the direction of NGC 2024

Details Radio recombination lines from carbon and heavier elements from the direction of NGC 2024 Radio recombination lines from carbon and heavier elements from the direction of NGC 2024

Nov 1974

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1974hrgc.conf..121h&link_type=abstract

H II regions and the galactic centre : proceedings of the Eighth ESLAB Symposium, 4-7 June 1974, Frascati, Italy, p. 121-123 (SE

Astronomy and Astrophysics

Astronomy

Carbon, Line Spectra, Nebulae, Radio Astronomy, Recombination Reactions, Emission Spectra, Hydrogen Clouds, Radio Telescopes, Superhigh Frequencies

Scientific paper

Observations of the 166 alpha line are reported in order to confirm
previous recombination line emissions which could correspond to an
element or elements with mass greater than carbon in the 157 alpha and
158 alpha (18 cm wavelength) radio recombination lines.

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