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Pulsation Properties of a Sample of Mira and OH/IR Stars

Published online by Cambridge University Press:  12 April 2016

M. J. Gaylard  and
M. E. West
M. J. Gaylard
Affiliation:
Hartebeesthoek Radio Astronomy Observatory, P O Box 443, Krugersdorp 1740, South Africa
M. E. West
Affiliation:
Hartebeesthoek Radio Astronomy Observatory, P O Box 443, Krugersdorp 1740, South Africa

Abstract

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Well-sampled light curves have been obtained for 1612-MHz hydroxyl masers in Mira and OH/IR stars monitored with the Hartebeesthoek radio telescope. Pulsation modes are investigated via the ratios of the observed periods in the maser variations.

Type
Part 2. Poster Papers
Information
International Astronomical Union Colloquium , Volume 155: Astrophysical Applications of Stellar Pulsation , 1995 , pp. 411 - 412
Copyright
Copyright © Astronomical Society of the Pacific 1995

References

Ostlie, D.A., & Cox, A.N. 1986, ApJ, 311, 864 CrossRefGoogle Scholar
Scargle, J.D. 1982, ApJ, 263, 835 Google Scholar
van Langevelde, H.J., van der Heiden, R., & van Schooneveld, C. 1990, A&A, 239, 193 Google Scholar
Wood, P.R. 1974, ApJ, 190, 609 CrossRefGoogle Scholar