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Structure of dense molecular gas in the TMC 1 from observations of three transitions of HC/sub 3/N

Journal Article · · Astrophys. J.; (United States)
DOI:https://doi.org/10.1086/160854· OSTI ID:5831348
We present high spatial resolution maps of the J = 5..-->..4, J = 9..-->..8, and J = 12..-->..11 transitions of HC/sub 3/N toward the interstellar cloud TMC 1 obtained with the Five College Radio Astronomy Observatory 14 m antenna. These transitions trace the high density molecular gas; the maps show that the dense material in TMC 1 is confined to a narrow ridge roughly 12' x 3' in extent. Maps of the source at individual velocities suggest that the ridge material is further divided into fragments which are in relative motion. The data are fitted to a cylindrical source model to determine the density and HC/sub 3/N column density within the ridge. The total mass of TMC 1 is approx.30 M/sub sun/, with each of the smaller fragments containing a few solar masses. The intensities of all three transitions are consistent with a single density of 5--10 x 10/sup 4/ cm/sup -3/; no variations in the density along the ridge are required by the data. The abundance of HC/sub 3/N in the models varies by approximately a factor of 3, from 10/sup -9/ at the cyanopolyne peak at the SE end of the ridge to 3 x 10/sup -10/ at the NH/sub 3/ peak to the NW. The present structure of TMC 1 probably resulted from the collapse and fragmentation of Heiles Cloud 2 and may eventually lead to the formation of stars.
Research Organization:
Five College Radio Astronomy Observatory, Department of Physics and Astronomy, University of Massachusetts, Amherst
OSTI ID:
5831348
Journal Information:
Astrophys. J.; (United States), Journal Name: Astrophys. J.; (United States) Vol. 267:1; ISSN ASJOA
Country of Publication:
United States
Language:
English

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