Dense Cores In The Serpens Molecular Cloud

Details Dense Cores In The Serpens Molecular Cloud Dense Cores In The Serpens Molecular Cloud

Dec 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992aas...181.4809f&link_type=abstract

American Astronomical Society, 181st AAS Meeting, #48.09; Bulletin of the American Astronomical Society, Vol. 24, p.1200

Astronomy and Astrophysics

Astronomy

1

Scientific paper

Submillimeter observations of the Serpens star forming region are presented. Recent CS 5--4 and 7--6 maps made with the Caltech Submillimeter Observatory show dense cores associated with both SVS-20 and FIRS-1 and an additional core near SVS-20 which is probably associated with a near by nebulous object. There is evidence for velocity gradients in these cores. CO 2-1 maps show the presence of broad lines with a complicated velocity field over much of the region around SVS-20 and FIRS-1. Maps made using the JCMT show a continuuum source associated with each dense core.

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