The channel maps and the position-velocity diagrams of multi-core structure of Cepheus C.

Details The channel maps and the position-velocity diagrams of multi-core structure of Cepheus C. The channel maps and the position-velocity diagrams of multi-core structure of Cepheus C.

Dec 1999

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1999pyuno....s.217y&link_type=abstract

Publications of the Yunnan Observatory, Suppl. 1999, p. 217 - 220

Physics

Protostellar Clouds: Structure

Scientific paper

The first important problem in the star forming process is the formation of proto-star core in star forming regions of molecular cloud. The multi-core structure in star forming regions is related to the forming of proto-star core. The molecular radiation of C18O (J = 1-0) in Cepheus C has been observed. The observations form the basis for an interesting study on the cloud cores and star formation activity. In order to study the multi-core structue the channel maps and the position-velocity diagrams will be shown. From the maps it is found that the contour level and distribution size of the three cores in Cepheus C are related to the channel velocity very much.

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