VLBI studies of the OH maser in W33

Details VLBI studies of the OH maser in W33 VLBI studies of the OH maser in W33

May 1987

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987pazh...13..399v&link_type=abstract

Pis'ma v Astronomicheskii Zhurnal (ISSN 0320-0108), vol. 13, May 1987, p. 399-405. In Russian. In Russian. In Russian.

Astronomy and Astrophysics

Astronomy

Hydroxyl Emission, Interstellar Masers, Very Long Base Interferometry, Amplitudes, Astronomical Maps, Brightness Temperature, Circular Polarization, Flux Density

Scientific paper

The OH maser in W33 was investigated at a frequency of 1665 MHz in left circular polarization by the Effelsberg-Onsala and Evapatoria-Simeiz-Pushchino radio interferometers. A map of the source was obtained; the angular sizes of the separate components were determined in the Gaussian approximation; and the flux densities and brightness temperatures of these components were measured.

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