A continuum and recombination line study of the CEP IV star formation region

Details A continuum and recombination line study of the CEP IV star formation region A continuum and recombination line study of the CEP IV star formation region

Jun 1980

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1980aj.....85..716r&link_type=abstract

Astronomical Journal, vol. 85, June 1980, p. 716-723.

Astronomy and Astrophysics

Astronomy

9

Centimeter Waves, Cepheid Variables, Continuous Spectra, Hydrogen Recombinations, Radio Astronomy, Star Formation, Frequency Distribution, H Ii Regions, Line Spectra, Stellar Spectra, Stellar Structure, Velocity Distribution

Scientific paper

The Cep IV star formation region consists of the Cep IV OB association, the H II regions W 1 and NGC 7822, and an extensive fragmented dust cloud complex. Six- and nine-cm radio continuum observations and 6-cm hydrogen recombination line observations show that all of the emission nebulosity in this region, which includes a large loop-type structure suggested by Herbst and Assousa (1977) to be a supernova remnant, has a thermal spectrum. The two components of W 1 have been detected at H 110 alpha and are found to be kinematically distinct.

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