Astronomy and Astrophysics – Astronomy
Scientific paper
Dec 1997
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1997apj...490..819g&link_type=abstract
Astrophysical Journal v.490, p.819
Astronomy and Astrophysics
Astronomy
7
Radio Lines: Stars, Stars: Carbon, Stars: Circumstellar Matter, Stars: Individual Alphanumeric: Irc +10216
Scientific paper
Five rotational transitions of vibrationally excited SiC2 in the nu 3 = 1 antisymmetric mode were sought toward IRC+10216: 414-313, 515-414, 615-514, 717-616, and 735-634. All five spectra show emission features. However, the 515-414 and 735-634 transitions are noticeably lower in intensity compared to the other three. In addition, the 414-313, 615-514, and 717-616 transitions have wider line widths than expected. For these reasons, we conclude that our detection of vibrationally excited SiC2 is tentative. The ratio of column densities of vibrationally excited SiC2 to ground state SiC2 is N( nu 3 = 1)/N( nu 3 = 0) <~ 0.024.
Gensheimer Paul David
Snyder Lewis E.
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