Interstellar Carbon Monosulfide

1971140 citationsJournal Article

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Abstract

We have observed line emission from the 146969.16-MHz j = 3 to j = 2 transition in CS in four sources. Typical column densities are near 1014 molecules cm . The excitation rates required to produce the observed line intensities are used to derive densities for the central regions of the sources.

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Spectroscopy and Laser Applications Atmospheric Ozone and Climate Astrophysics and Star Formation Studies

Publication Details

Published in: The Astrophysical Journal

Volume 168, pp. L53-L53

DOI: 10.1086/180784

Field-Weighted Citation Impact: 5.04

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Interstellar Carbon Monosulfide

Authors

Abstract

Topics & Keywords

Publication Details