Astronomy and Astrophysics – Astronomy
Scientific paper
Mar 1978
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1978apj...220..500c&link_type=abstract
Astrophysical Journal, Part 1, vol. 220, Mar. 1, 1978, p. 500, 501, 503-509. Research supported by the University of Kentucky a
Astronomy and Astrophysics
Astronomy
12
Condensation, Interstellar Gas, Molecular Spectra, Nebulae, Radio Sources (Astronomy), Angular Momentum, Cores, Gas Spectroscopy, Line Spectra
Scientific paper
A small region around the high-density core of the optical condensation referred to as B213 NW has been studied in some detail. The 2-cm formaldehyde spectral line was used as a probe for the study. The gas in this region is observed to consist of several fragments, the most massive of which appears to be rotating. The other fragment observed with the 2-cm line appears to be unbound and will escape from B213 NW. The relationship between the gas in this dense core and the parent cloud is discussed. A method of determining the distance to dense gas clouds which exhibit rotation is outlined.
Clark Frank O.
Johnson Richard D.
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