High angular resolution observations of CS in the Orion nebula

Details High angular resolution observations of CS in the Orion nebula High angular resolution observations of CS in the Orion nebula

Sep 1980

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1980apj...240..524g&link_type=abstract

Astrophysical Journal, Part 1, vol. 240, Sept. 1, 1980, p. 524-531.

Astronomy and Astrophysics

Astrophysics

43

Carbon Compounds, Emission Spectra, Molecular Clouds, Orion Nebula, Protostars, Sulfides, Angular Resolution, Electron Transitions, Interstellar Matter

Scientific paper

The core of the Orion molecular cloud has been observed in the emission lines of CS at 146.8 and 97.98 GHz, using the 14 m FCRAO telescope. The morphology indicated by these new data, combined with previous observations, is an extremely narrow ridge extending 9 min N-S as well as a central condensation at the position of the Kleinmann-Low nebula. Within the central condensation the observations show no evidence of significant clumping on the scale of the beam despite the high sensitivity of this transition to changes in H2 density.

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