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Kinematic Evidence For Fundamental Mode Pulsation in the Short-Period Classical Cepheid SU Cassiopeiae

Published online by Cambridge University Press:  12 April 2016

D. G. Turner ,
D. W. Forbes ,
R. W. Lyons  and
R. J. Havlen
D. G. Turner
Affiliation:
Saint Mary's University, Halifax, NS, B3H 3C3, Canada
D. W. Forbes
Affiliation:
Trent University, Peterborough, Ont., K9J 7B8, Canada
R. W. Lyons
Affiliation:
David Dunlap Observatory
R. J. Havlen
Affiliation:
N.R.A.O.

Extract

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The short period and small amplitude of pulsation for the 1d.95 Cepheid SU Cas make it an excellent candidate for pulsation in a purely excited mode, and, as summarized by Gieren (1982), there is some evidence from recent radius determinations for this variable which suggests that it is indeed an overtone pulsator.

Type
Part I. Fundamental Parameters
Information
International Astronomical Union Colloquium , Volume 82: Cepheids: Theory and Observations , 1985 , pp. 95 - 97
Copyright
Copyright © Cambridge University Press 1985

References

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van den Bergh, S. (1977). IAU Colloq. 37, 13.Google Scholar