Search for (C-12)O emission at high galactic latitude

Details Search for (C-12)O emission at high galactic latitude Search for (C-12)O emission at high galactic latitude

Dec 1983

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983aj.....88.1832d&link_type=abstract

Astronomical Journal (ISSN 0004-6256), vol. 88, Dec. 1983, p. 1832-1834. NSF-supported research.

Astronomy and Astrophysics

Astronomy

2

Carbon Monoxide, Hydrogen Clouds, Interstellar Extinction, Microwave Emission, Milky Way Galaxy, Interstellar Matter, Millimeter Waves

Scientific paper

The authors searched for 12CO emission from several regions at high galactic latitude. The observed regions were chosen because they showed both high H I column density and relatively low galaxy counts, suggesting the possible presence of obscuring material. No CO emission was detected at a 4σ level of 0.28K antenna temperature. This result does not rule out the presence of obscuring material but does place some limitations on the nature of the regions observed.

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