Constraints on the molecular properties of interstellar X-ogen derived from radio observations

Details Constraints on the molecular properties of interstellar X-ogen derived from radio observations Constraints on the molecular properties of interstellar X-ogen derived from radio observations

Sep 1975

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1975apj...200..584h&link_type=abstract

Astrophysical Journal, vol. 200, Sept. 15, 1975, pt. 1, p. 584-593.

Other

28

Interstellar Matter, Line Spectra, Molecular Spectra, Radio Spectra, Spectrum Analysis, Electron Transitions, Graphs (Charts), Tables (Data)

Scientific paper

Twenty-eight X-ogen emission sources at 89.189 GHz have been detected and observed. Twenty of these are new X-ogen sources which also contain other interstellar molecules. No infrared stars are found to be X-ogen sources. A new rest frequency (89,188.65 MHz) is derived for X-ogen. It is shown that X-ogen is not SiC, C2H, or any molecule with spin-doubling, hyperfine structure, or both.

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