On the identification of molecules in the cool carbon stars

Details On the identification of molecules in the cool carbon stars On the identification of molecules in the cool carbon stars

Oct 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988pasp..100.1202l&link_type=abstract

Astronomical Society of the Pacific, Publications (ISSN 0004-6280), vol. 100, Oct. 1988, p. 1202-1215. Research supported by the

Astronomy and Astrophysics

Astronomy

12

Carbon Stars, Cool Stars, Molecular Spectra, Stellar Spectra, Asymptotic Giant Branch Stars, Emission Spectra, Spectral Line Width, Stellar Evolution

Scientific paper

Various problems encountered in identifying molecular lines in the rich spectra of cool carbon and related stars are considered. Special attention is given to the FeH, ZrS, and CN molecules. Following a review of the principles of identifying stellar lines, recent successful identifications are discussed that illustrate the wide range in the incompleteness of the laboratory spectroscopy.

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