Observations of young stellar clusters in the 18-cm OH lines

Details Observations of young stellar clusters in the 18-cm OH lines Observations of young stellar clusters in the 18-cm OH lines

Apr 1978

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1978sva....22..199r&link_type=abstract

(Astronomicheskii Zhurnal, vol. 55, Mar.-Apr. 1978, p. 345-349.) Soviet Astronomy, vol. 22, Mar.-Apr. 1978, p. 199-201. Transla

Astronomy and Astrophysics

Astronomy

Centimeter Waves, Hydroxyl Emission, Line Spectra, Radio Astronomy, Star Clusters, Microwave Emission, Radio Stars, Stellar Radiation

Scientific paper

In 1974-1975 observations of 12 young galactic star clusters and associations were conducted in the 1667- and 1665-MHz lines of the ground state of the OH molecule. The 1667-MHz emission was detected in the Cep OB IV association. Besides that, the 1667-MHz emission was observed at several points in the cluster NGC 2264. For the remaining clusters, upper limits on the intensity of OH emission have been determined, the antenna temperature being less than 0.15-0.25 K.

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