Compact continuum radio sources in the Orion Nebula

Details Compact continuum radio sources in the Orion Nebula Compact continuum radio sources in the Orion Nebula

Oct 1982

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982nyasa.395..204m&link_type=abstract

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

Astronomy and Astrophysics

Astronomy

7

Hydrogen Clouds, Molecular Clouds, Orion Nebula, Radio Sources (Astronomy), Astronomical Maps, Flux Density, Masers, Radio Astronomy, Radio Spectra

Scientific paper

The authors observed the Orion Nebula with the VLA searching for compact radio sources that would help establish which of the infrared sources in the Becklin-Neugebauer-Kleinmann-Low (BN-KL) region might contain primary energy sources. They detected radio emission from the BN object at 15 and 23 GHz. No emission was found from IRc2, which is thought to be the source of the flow that gives rise to maser emission. In addition, the authors detected ten compact sources associated with the Trapezium cluster and four other sources near the molecular cloud.

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