Aperture synthesis observations of Orion B at 2.695 and 8.085 GHz

Details Aperture synthesis observations of Orion B at 2.695 and 8.085 GHz Aperture synthesis observations of Orion B at 2.695 and 8.085 GHz

Apr 1983

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983a%26a...120..322w&link_type=abstract

Astronomy and Astrophysics (ISSN 0004-6361), vol. 120, no. 2, April 1983, p. 322-325.

Astronomy and Astrophysics

Astronomy

5

Radio Sources (Astronomy), Astronomical Maps, H Ii Regions, Interferometry, Microwave Emission, Synthetic Apertures

Scientific paper

Interferometer observations of Orion B at 2.695 and 8.085 GHz are presented. Orion B appears to be a double source: one H II region associated with the star NGC 2024 No. 2 and an extended H II region surrounding the star NGC 2024 No. 1. This structure gives support to the model that the stars NGC 2024 No. 2 and No. 1 (of spectral type O 9.5 and B 0.5, respectively) ionize the nebula.

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