Absorption of OH in the direction toward the galactic center

Details Absorption of OH in the direction toward the galactic center Absorption of OH in the direction toward the galactic center

Aug 1974

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1974azh....51..681l&link_type=abstract

Astronomicheskii Zhurnal, vol. 51, July-Aug. 1974, p. 681-684. In Russian.

Astronomy and Astrophysics

Astronomy

Absorption Spectra, Cloud Physics, Galactic Nuclei, Hydroxyl Emission, Milky Way Galaxy, Radio Astronomy, Computer Techniques, Interstellar Extinction, Interstellar Matter, Microwave Emission, Optical Thickness

Scientific paper

High angular and spectral resolution observations of the OH 1167 MHz
absorption line performed with a radio telescope at Nancay, France, are
discussed. Among the six OH clouds detected is a cloud with a radial
velocity of +40 km/sec. It is shown that the latter cloud can be
resolved into two components. The structure of the cloud is analyzed.

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