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Title:
Molecular clouds around outflow sources
Authors:
Verdes-Montenegro, L.; Torrelles, J. M.; Rodriguez, L. F.; Anglada, G.; Lopez, R.
Affiliation:
AA(Andalucia, Instituto de Astrofisica, Granada, Spain), AB(Andalucia, Instituto de Astrofisica, Granada, Spain), AC(Universidad Nacional Autonoma de Mexico, Coyoacan, Mexico), AD(Barcelona, Universidad, Spain), AE(Barcelona, Universidad, Spain)
Publication:
(IAU, European Regional Astronomy Meeting, 11th, La Laguna, Spain, July 3-8, 1989) Astrophysics and Space Science (ISSN 0004-640X), vol. 171, no. 1-2, Sept. 1990, p. 161, 162. (Ap&SS Homepage)
Publication Date:
09/1990
Category:
Astrophysics
Origin:
STI
NASA/STI Keywords:
AMMONIA, EMISSION SPECTRA, GAS FLOW, MOLECULAR CLOUDS, STAR FORMATION, CARBON MONOXIDE, STELLAR EVOLUTION
DOI:
10.1007/BF00646838
Bibliographic Code:
1990Ap&SS.171..161V

Abstract

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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