CS observations of selected star-forming regions

Details CS observations of selected star-forming regions CS observations of selected star-forming regions

Jun 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989ap%26ss.156..251b&link_type=abstract

(Instituto de Astrofisica de Canarias and Comision Interministerial de Ciencia y Tecnologia, Summer School on Evolutionary Pheno

Astronomy and Astrophysics

Astrophysics

1

Carbon Compounds, Molecular Clouds, Star Formation, Sulfides, Ammonia, Emission Spectra, Herbig-Haro Objects, Nebulae, T Tauri Stars

Scientific paper

Maps of the CS (J = 1-0) emission at 49 GHz of L43 (RNO 91), NGC 2068 (HH 19-27) and L1524 (Haro 6-10) are presented. Physical parameters of these clouds are derived from the observations. The CS emission is compared with ammonia emission maps obtained with a similar angular resolution. Both CS and ammonia molecules are tracers of the high-density gas in molecular clouds. Thus, a similar distribution of the emission is expected. However, these observations show evidence of some remarkable morphological differences.

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