SO and CS observations of molecular clouds. I. The observational data

Details SO and CS observations of molecular clouds. I. The observational data SO and CS observations of molecular clouds. I. The observational data

Jun 2000

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2000a%26as..144..441n&link_type=abstract

Astronomy and Astrophysics Supplement, v.144, p.441-450

Astronomy and Astrophysics

Astrophysics

1

Ism: Clouds, Ism: Molecules

Scientific paper

We present in this article a rather extensive mapping survey of 19 Galactic molecular clouds in the CS(J=2-1) and SO(J_N=3_2-2_1) lines using the Onsala 20 m telescope. The data, taken with the same angular resolution of ~ 40'', are presented as integrated intensity maps and for some relevant positions we also present spectra of the previously mentioned lines and their 34S substituted isotopomer lines. For map positions where we have observed at least one of the less abundant isotopomer transitions we have tabulated the integrated intensities of all observed transitions (\tref{t:IntInt}). Already a visual inspection of the maps reveals considerable differences between the SO and CS integrated intensity distributions. Figs. 1 to 9 are only available at http://www.edpsciences.org

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