Time Monitoring of SiO (v=1, J=2-1) Maser Emission from Late Type Stars

Details Time Monitoring of SiO (v=1, J=2-1) Maser Emission from Late Type Stars Time Monitoring of SiO (v=1, J=2-1) Maser Emission from Late Type Stars

Jul 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985mlrg.proc..223n&link_type=abstract

Mass Loss from Red Giants; Proceedings of the Conference, University of California, Los Angeles, CA, June 20, 21, 1984. Edited

Astronomy and Astrophysics

Astrophysics

1

Scientific paper

The time variations of the SiO (υ = 1, J = 2-1) maser line towards eight late type stars have been observed with the Onsala 20 m telescope. Long-term changes of the total width and centre velocity of the SiO lines can be seen in some of the sources. The best example is ο Ceti where the centre velocity has increased steadily from 45 to 50 km s-1 from 1978 to 1984. This may be an effect of ο Ceti being a binary stars.

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