The galaxy's 157 micron (C 2) emission: Observations by means of a spectroscopic lunar-occultation technique

Details The galaxy's 157 micron (C 2) emission: Observations by means of a spectroscopic lunar-occultation technique The galaxy's 157 micron (C 2) emission: Observations by means of a spectroscopic lunar-occultation technique

Apr 1983

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983asnyn...2...20s&link_type=abstract

News Lett. Astron. Soc. N. Y., Vol. 2, No. 3, p. 20

Astronomy and Astrophysics

Astronomy

Galactic Radiation, Lunar Occultation, Spectroscopy, Fine Structure, Interstellar Matter, Radiation Detectors

Scientific paper

Galactic (C II) 157 micron, fine-structure emission was estimated. At a
Galactic longitude of 8 deg, the peak power observed in a 7' x 7' field
is approx. 5 x 10 to the -9 Watt. The method used to detect this
radiation involved chopping against the cold side of the Moon.

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