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A Polarization Model for 12 Lacertae

Published online by Cambridge University Press:  25 April 2016

P. A. Stamford  and
R. D. Watson
P. A. Stamford
Affiliation:
Department of physics, University of Tasmania
R. D. Watson
Affiliation:
Department of physics, University of Tasmania
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Extract

Recent evidence suggests that radial pulsation can explain most of the variability in the majority of well-studied β Cephei stars (Stamford and Watson 1978; Campos and Smith 1980).

Type
Contributions
Information
Publications of the Astronomical Society of Australia , Volume 4 , Issue 1 , 1980 , pp. 83 - 85
Copyright
Copyright © Astronomical Society of Australia 1980

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References

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