Infrared observation of NGC 6334

Details Infrared observation of NGC 6334 Infrared observation of NGC 6334

Nov 1974

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1974hrgc.conf...39b&link_type=abstract

H II regions and the galactic centre : proceedings of the Eighth ESLAB Symposium, 4-7 June 1974, Frascati, Italy, p. 39-42 (SEE

Astronomy and Astrophysics

Astronomy

21

Infrared Spectrophotometers, Mapping, Nebulae, Hydrogen Clouds, Infrared Astronomy, Radiation Sources, Silicates

Scientific paper

Infrared photometric observations of three components in NGC 6334 were made. Two of the components are associated with compact H2 regions and are similar to the sources in W3. The third component is almost coincident with the OH maser source and shows no known radio continuum emission. A component of the infrared emitting region is less than 1 inch in diameter at 10 microns and shows a strong silicate dust absorption feature. In many respects, this source is very similar to the BN infrared source in the Orion nebula.

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