Molecular clouds around outflow sources

Details Molecular clouds around outflow sources Molecular clouds around outflow sources

Sep 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990ap%26ss.171..161v&link_type=abstract

(IAU, European Regional Astronomy Meeting, 11th, La Laguna, Spain, July 3-8, 1989) Astrophysics and Space Science (ISSN 0004-640

Astronomy and Astrophysics

Astrophysics

Ammonia, Emission Spectra, Gas Flow, Molecular Clouds, Star Formation, Carbon Monoxide, Stellar Evolution

Scientific paper

The (J, K) = (1, 1) ammonia transition emission has been observed toward six regions with signs of active star formation (AFGL 5142, HH 33/40, AFGL 5157, AFGL 6366S, HHL 73, and S140N), using the 37-m antenna of the Haystack Observatory. The ammonia emission was detected and mapped in all of these sources with the exception of HH 33/40. The (J, K) = (2, 2) ammonia transition was also observed at the peak position of each source in order to obtain the rotational temperature of the ammonia clumps.

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