Ammonia Study Of The High-Mass Star-Forming Region G111.6+0.3

Details Ammonia Study Of The High-Mass Star-Forming Region G111.6+0.3 Ammonia Study Of The High-Mass Star-Forming Region G111.6+0.3

May 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010aas...21642411l&link_type=abstract

American Astronomical Society, AAS Meeting #216, #424.11; Bulletin of the American Astronomical Society, Vol. 41, p.837

Physics

Scientific paper

Observations of the UC HII region G111.61+0.3, and its associated PDR, suggest that a hot molecular core may be present, and nearby coincident with the arc of the cometary HII region. The NH3(3,3) and NH3(4,4) were observed in order to determine the presence of a hot molecular core. This observations also give us the opportunity to study physics of the interaction between ionized, neutral and molecular gas components. Here we present the results of this ammonia study.

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