CO velocity features in the Orion molecular cloud associated with shock fronts and expansion of the Orion H II region

Details CO velocity features in the Orion molecular cloud associated with shock fronts and expansion of the Orion H II region CO velocity features in the Orion molecular cloud associated with shock fronts and expansion of the Orion H II region

Dec 1979

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1979apj...234l.207l&link_type=abstract

Astrophysical Journal, Part 2 - Letters to the Editor, vol. 234, Dec. 15, 1979, p. L207-L211.

Astronomy and Astrophysics

Astronomy

26

Carbon Monoxide, H Ii Regions, Interstellar Gas, Molecular Gases, Orion Nebula, Millimeter Waves, Radio Astronomy, Shock Fronts

Scientific paper

Kinematic features of CO and (C-13)O are identified with an expanding
shock advancing into the neutral gas surrounding the Orion H II region.
Expansion is shown to be retarded by the presence of several distinct
dense neutral clouds in the vicinity of the H II region. Several new CO
hot spots are likely candidates for embedded infrared sources.

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