HCO(+) and SO emission associated with the region G34.3+0.2

Details HCO(+) and SO emission associated with the region G34.3+0.2 HCO(+) and SO emission associated with the region G34.3+0.2

May 1987

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987rmxaa..14..506c&link_type=abstract

(IAU, Reunion Regional Latinoamericana de Astronomia, 5th, Merida, Mexico, Oct. 6-10, 1986) Revista Mexicana de Astronomia y Ast

Astronomy and Astrophysics

Astronomy

6

Formyl Ions, H Ii Regions, Hydroxyl Emission, Interstellar Masers, Radio Astronomy, Sulfur Oxides, High Resolution, Microwave Emission, Molecular Clouds, Morphology, Stellar Winds

Scientific paper

The authors have used the Hat Creek millimeter interferometer to map the 89.1 GHz and 86.1 GHz lines of HCO+ and SO in the direction of the H II region G34.3+0.2. The spatial distribution and the measured velocity of the HCO+ core, support the "champagne phase" model for the compact H II region. A broad (≡20 km s-1) HCO+ absorption is detected towards the compact H II region. This suggests the presence of a young object close to the H II region that is producing an outflow.

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