An Unusual Burst of OH Maser Emission in the Source Vy-Canis

Details An Unusual Burst of OH Maser Emission in the Source Vy-Canis An Unusual Burst of OH Maser Emission in the Source Vy-Canis

Jun 1986

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986pazh...12..361y&link_type=abstract

Pis'ma v Astronomicheskii Zhurnal, Vol. 12:5, P. 361, 1986

Astronomy and Astrophysics

Astronomy

1

Scientific paper

Results of observations of the source VY CMa, made from May 1983 to April 1985 with the RATAN-600 radio telescope in the main lines of the OH maser emission 1665 and 1667 MHz are described. In February - March 1985 the burst of OH maser emission occurred, which was accompanied by symmetrical satellite details and strong flux variation of the main component of the emission profile. The probable geometry of maser emission region is discussed.

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