Observations of the young stellar association ON2

Details Observations of the young stellar association ON2 Observations of the young stellar association ON2

Dec 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988mnras.235.1397d&link_type=abstract

Monthly Notices of the Royal Astronomical Society (ISSN 0035-8711), vol. 235, Dec. 15, 1988, p. 1397-1410. Research supported by

Astronomy and Astrophysics

Astronomy

17

Early Stars, Far Infrared Radiation, Molecular Clouds, Star Formation, Ammonia, Cosmic Dust, Emission Spectra, Gas Temperature, H Ii Regions, Interstellar Masers

Scientific paper

Results are presented from a study of the star-formation region ON2 in molecular lines and the far-infrared. Ammonia maps of the dense gas show a double structure, with young stars located around the cloud edges. Localized heating of the molecular gas is evident near these early-type stars, and molecular hydrogen densities of ≈105cm-3 are required to maintain the observed gas temperature through gas/dust coupling.

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