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The Variable Polarization of T Cen

Published online by Cambridge University Press:  25 April 2016

A. Victoria Peterson
A. Victoria Peterson*
Affiliation:
Mount Stromlo and Siding Spring Observatories, The Australian National University, Canberra
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Extract

T Centauri (HD119090) is a semi-regular variable with a period of 90d.61. The period is apparently stable but the photometry does not repeat very closely from cycle to cycle. The general Catalogue of Variable Stars gives a range of magnitudes from 5.5 to 9.0 and spectral types from KOe to M4IIe.

Type
Contributions
Information
Publications of the Astronomical Society of Australia , Volume 2 , Issue 2 , March 1972 , pp. 108 - 110
Copyright
Copyright © Astronomical Society of Australia 1972

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References

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