Radio Continuum Emission from the CEPHEUS-OB3 Molecular Cloud Infrared Source

Details Radio Continuum Emission from the CEPHEUS-OB3 Molecular Cloud Infrared Source Radio Continuum Emission from the CEPHEUS-OB3 Molecular Cloud Infrared Source

Feb 1981

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1981a%26a....94..231h&link_type=abstract

Astronomy and Astrophysics, Vol. 94, P. 231, 1981

Astronomy and Astrophysics

Astrophysics

15

Scientific paper

Regions A and F of the giant CO cloud Cepheus OB 3 are observed in the radio continuum at 0.6, 4.8, 10.7, and 14.7 GHz. Four sources are detected, two of which are compact H II regions. One of these is located at the position of maximum CO emission from region A which may be a complex site of current star formation, containing several sources at different evolutionary stages. The other H II region detected lies at an extension of the CO region F.

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