Probing the possibility of a (12)C/(13)C abundance gradient from observations of interstellar CH+

Details Probing the possibility of a (12)C/(13)C abundance gradient from observations of interstellar CH+ Probing the possibility of a (12)C/(13)C abundance gradient from observations of interstellar CH+

Sep 1987

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987acs..meet.....h&link_type=abstract

Presented at the 194th American Chemical Society National Meeting, New Orleans, La., 31 Aug. - 4 Sep. 1987

Physics

Abundance, Carbon 12, Carbon 13, Gradients, Interstellar Matter, Methane, Radicals, Hydrogen, Interstellar Space

Scientific paper

High signal-to-noise (S/N= 300 to 500) observations have been performed
of interstellar CH(+) at Lick Observatory and at CTIO of the reddened,
early-type stars HD 183143, HD 24432, and HD 157038 in an effort to
probe the existence of a C-12/C-13 abundance gradient in our Galaxy.

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