On the interpretation of the broad-band millimeter-wave flux from Orion

Details On the interpretation of the broad-band millimeter-wave flux from Orion On the interpretation of the broad-band millimeter-wave flux from Orion

Aug 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984apj...283l..41s&link_type=abstract

Astrophysical Journal, Part 2 - Letters to the Editor (ISSN 0004-637X), vol. 283, Aug. 15, 1984, p. L41-L44.

Astronomy and Astrophysics

Astronomy

59

Millimeter Waves, Molecular Clouds, Orion Nebula, Radio Astronomy, Broadband, Emission Spectra, Flux Density

Scientific paper

Spectral observations of the core of Orion A at wavelengths around 1.3 mm show a high density of strong, broad emission lines. The combined flux in lines with peak antenna temperatures stronger than 0.2 K accounts for approximately 40 percent of the broad-band millimeter-wave flux from the region. Thus the broad-band flux from Orion A is in large part due to sources other than dust emission.

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