Synthesis observations of the radio continuum radiation of the H II region NGC 7822 /W1/

Details Synthesis observations of the radio continuum radiation of the H II region NGC 7822 /W1/ Synthesis observations of the radio continuum radiation of the H II region NGC 7822 /W1/

Nov 1981

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1981a%26a...103...50h&link_type=abstract

Astronomy and Astrophysics, vol. 103, no. 1, Nov. 1981, p. 50-56.

Astronomy and Astrophysics

Astronomy

7

Astronomical Maps, H Ii Regions, Radio Astronomy, Stellar Evolution, Angular Resolution, Early Stars, H Alpha Line, Ionizing Radiation, Spectrum Analysis, Star Clusters, Stellar Radiation

Scientific paper

New observations of the W1 complex made at 0.6, 1.4, and 5.0 GHz using the Westerbork Synthesis Radio Telescope are reported. The main goal of the observations was to study the small scale structure of the H II region with angular resolutions ranging from 7 to 56 arcsec. The radio data are consistent with the hypothesis that NGC 7822 (W1) is an evolved H II region at a distance of 850 pc. Observations also suggest the presence of additional ionizing stars in both G118.6+4.8 and G118.1+5.0.

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