Millimeter-wavelength lines from the Orion plateau source

Details Millimeter-wavelength lines from the Orion plateau source Millimeter-wavelength lines from the Orion plateau source

Oct 1982

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982nyasa.395..100k&link_type=abstract

(NASA, National Science Foundation, New York Academy of Sciences, et al., Symposium on the Orion Nebula to Honor Henry Draper, N

Other

Carbon Monoxide, Emission Spectra, Line Spectra, Millimeter Waves, Molecular Clouds, Orion Nebula, Gas Flow, Interstellar Chemistry, Interstellar Matter, Stellar Evolution

Scientific paper

Emission lines from molecules in the Orion Molecular Cloud have a two-component structure; a "spike" feature superposed upon a broader "plateau" feature, with both components being centered at about the same velocity. The plateau feature is confined to a region with a diameter of less than a minute of arc centered on the BN-KL cluster. The present review deals with the observed properties of the plateau component. The available evidence on the position, size, mass, energy, and composition is summarized and the properties of the source are compared with those of other sources and with speculations about the origin and nature of the source.

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