Wide beam measurements of H2 regions in the infrared

Details Wide beam measurements of H2 regions in the infrared Wide beam measurements of H2 regions in the infrared

Nov 1974

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1974hrgc.conf...53l&link_type=abstract

H II regions and the galactic centre : proceedings of the Eighth ESLAB Symposium, 4-7 June 1974, Frascati, Italy, p. 53-59 (SEE

Astronomy and Astrophysics

Astronomy

Far Infrared Radiation, Hydrogen Clouds, Infrared Astronomy, Nebulae, Beams (Radiation), Brightness, Cosmic Dust, Hydrogen Ions, Mapping, Radio Emission

Scientific paper

Several of the brighter and more extended H 2 regions in the far infrared of the Omega nebula 1417 as seen at 21 micrometers were studied. For this type of observation, a small telescope can be used: most measurements were made with a 28 inch telescope, and occasionally a 60 inch was used. Because of the combination of the poor 21 micrometer window, large beam diameter, and a large chopper throw, sensitivity was severely limited by sky noise. Results in the form of contour maps and radio continuum maps are discussed.

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