Fine radio structure in W3

Details Fine radio structure in W3 Fine radio structure in W3

Mar 1976

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1976mnras.174..649h&link_type=abstract

Monthly Notices of the Royal Astronomical Society, vol. 174, Mar. 1976, p. 649-659.

Astronomy and Astrophysics

Astronomy

92

Fine Structure, Hydroxyl Emission, Interstellar Masers, Microwave Emission, Radio Sources (Astronomy), Astronomical Maps, H Ii Regions, Hydrogen Ions, O Stars, Radio Astronomy, Radio Emission, Telescopes

Scientific paper

The H II region W3 has been mapped at 5 GHz with 2-arcsec resolution
using the Cambridge 5-km telescope. Several new faint sources have been
detected. Analysis of the shell source W3(A) shows it to be excited by
two highly obscured O-stars and to be strongly ionization-bounded.

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