High angular resolution observations of the maser source W3(OH)

Details High angular resolution observations of the maser source W3(OH) High angular resolution observations of the maser source W3(OH)

May 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989pazh...15..407a&link_type=abstract

Pis'ma v Astronomicheskii Zhurnal (ISSN 0320-0108), vol. 15, May 1989, p. 407-412. In Russian.

Astronomy and Astrophysics

Astronomy

Hydroxyl Emission, Interstellar Masers, Radio Sources (Astronomy), Angular Resolution, Brightness Temperature, Maser Outputs, Radio Interferometers

Scientific paper

In February 1986, the maser source W3(OH) was observed with a radio
interferometer at 1665 MHz. It is found that the source has several
compact components with sizes in the range 4-10 AU and brightness
temperatures of about 10 to the 12th K.

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