Other
Scientific paper
Aug 1983
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983apj...271l..89j&link_type=abstract
Astrophysical Journal, Part 2 - Letters to the Editor (ISSN 0004-637X), vol. 271, Aug. 15, 1983, p. L89-L93.
Other
67
Centimeter Waves, Formaldehyde, Interstellar Matter, Molecular Clouds, Orion Nebula, Absorption Spectra, Continuous Spectra, Emission Spectra, H Ii Regions, Spectral Energy Distribution
Scientific paper
VLA observations of the H2CO 6 cm line associated with OMC-1 at a resolution of several arcsec are reported. Maps are constructed with dominant features from high-density regions. The dominant emission condensation is located near the Kleinmann-Low (KL) nebula and is centered near IRc5; it is 0.06 x 0.03 pc in size, and its peak main brightness of 9 K implies that the H2CO excitation is thermal. The dominant absorption condensation is approximately 2 arcmin south of KL and is 30 arcsec or less in size. Its peak brightness temperature is -5 K, from which it is inferred that the clump is probably behind the H II region. The other weaker absorption and emission features are consistent with sizes greater than 15 arcsec and show clumpy structures.
Bieging John H.
Johnston Ken J.
Palmer Patrick
Wilson Thomas L.
No associations
LandOfFree
The distribution of 6 centimeter H2CO in Orion Molecular Cloud 1 does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.
If you have personal experience with The distribution of 6 centimeter H2CO in Orion Molecular Cloud 1, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and The distribution of 6 centimeter H2CO in Orion Molecular Cloud 1 will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-741798