Absorption and emission by interstellar CH at 9 cm

Details Absorption and emission by interstellar CH at 9 cm Absorption and emission by interstellar CH at 9 cm

Mar 1974

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1974natur.248...31r&link_type=abstract

Nature, Volume 248, Issue 5443, pp. 31-32 (1974).

Physics

13

Scientific paper

RYDBECK, Ellder and Irvine1 have recently detected the 9-cm lines of the 2Pcy1/2, J = 1/2Λ doublet of interstellar CH. The F = 1 --> 1 transition at 3,335.475 MHz was observed in emission in a wide range of galactic sources ranging from dark clouds to the spiral arms in front of Cassiopea A. The two satellite transitions F = 0 --> 1 (at 3,263.788 MHz) and F 1 --> 0 (at 3,349.185 MHz) were also observed in emission in several sources.

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