Molecular outflows in the Serpens cloud core? - FIRS 1 and SVS 4

Details Molecular outflows in the Serpens cloud core? - FIRS 1 and SVS 4 Molecular outflows in the Serpens cloud core? - FIRS 1 and SVS 4

Apr 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992pasj...44..155e&link_type=abstract

PASJ: Publications of the Astronomical Society of Japan (ISSN 0004-6264), vol. 44, no. 2, 1992, p. 155-158. Research supported b

Astronomy and Astrophysics

Astronomy

7

Molecular Clouds, Molecular Flow, Pre-Main Sequence Stars, Star Formation, Astronomical Models, Carbon Monoxide, Molecular Gases

Scientific paper

The paper reports on CO(J = 1-0) high-velocity wing emission toward two young objects of the Serpens molecular cloud, FIRS 1 and SVS 4. These observations were carried out with the 45-m telescope of the Nobeyama Radio Observatory. Different kinds of CO wing profiles found toward these two regions suggest that the previously reported extended (not less than 6 arcmin) molecular outflow in the region is the result of perturbations on the ambient molecular gas by local outflows associated with various young objects.

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