Astronomy and Astrophysics – Astronomy
Scientific paper
May 1994
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1994aas...184.3003k&link_type=abstract
American Astronomical Society, 184th AAS Meeting, #30.03; Bulletin of the American Astronomical Society, Vol. 26, p.905
Astronomy and Astrophysics
Astronomy
Scientific paper
This study demonstrates a crucial difference between quiescent Bok globules and dark cloud cores. Seventeen small, quiescent Bok globules were probed for the molecular lines of NH_3 (J,K=1,1) and HC_3N (J=4->3) using the Haystack telescope. The sources have 3sigma integrated line intensity upper limits generally less than 0.1 K-km s(-1) . In terms of the reference source, TMC-2, this is less than about 10% of the brightness of the NH_3 (1,1) line, and less than about 30% of brightness of the HC_3N (4->3) line. A simple statistical equilibrium analysis indicates that chemical abundances of NH_3 and HC_3N in these globules are diminished by factors of 10 and 6, respectively, relative to dark cloud cores. Second, for plausible globule core sizes, densities are about 6 times smaller compared to those of dark cloud cores.
Clemens Dan P.
Kane Brian D.
Myers Phil C.
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