The New Observation of C 18O(J=1--0) Molecular Emission in the Cepheus OB3 Molecular Cloud

Details The New Observation of C 18O(J=1--0) Molecular Emission in the Cepheus OB3 Molecular Cloud The New Observation of C 18O(J=1--0) Molecular Emission in the Cepheus OB3 Molecular Cloud

Nov 1996

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1996apj...471..867y&link_type=abstract

Astrophysical Journal v.471, p.867

Astronomy and Astrophysics

Astronomy

6

Ism: Clouds, Ism: Molecules, Ism: Structure, Ism: Individual Name: Cepheus Ob3

Scientific paper

We present the C18O(J = 1-0) observation of the Cep OB3 molecular cloud. The observation was made for a week in 1993 December with the new 4 m millimeter telescope at Nagoya University. The extent of the C18O(J = 1-0) emission indicates that total area coverage of the map is substantially less than 2°.8 x 1°.4 structure. A portion of the Cep OB3 molecular cloud has been mapped in the C18O(J = 1-0) line on a completely sampled grid with a 2'.O spacing. The physical parameters of the C18O(J = 1-0) core are derived. The C18O(J = 1-0) emission is also tracing the dense gas in the core. The large dense core appears to have been disturbed significantly by the star formation activity within it.

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