Hot ammonia toward the H2O masers near W3(OH)

Details Hot ammonia toward the H2O masers near W3(OH) Hot ammonia toward the H2O masers near W3(OH)

Sep 1986

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986a%26a...166l..26m&link_type=abstract

Astronomy and Astrophysics (ISSN 0004-6361), vol. 166, no. 1-2, Sept. 1986, p. L26-L28.

Astronomy and Astrophysics

Astrophysics

9

Ammonia, Interstellar Masers, Molecular Clouds, Water Masers, H Alpha Line, H Ii Regions, High Temperature Gases, Hydrocyanic Acid, Recombination Reactions

Scientific paper

A map of the (J,K) = (5,5) line of NH3 toward the ultracompact H II region W3(OH), made with a 38arcsec beam, is presented. From the comparison of the absorption and emission lines of NH3 with H64α line data, the emission arises ≡8arcsec east of the continuum source and arises from the region where H2O and HCN emission is observed. This gas is probably heated by an embedded source with a luminosity ≥104L_sun;.

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