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Period Changes in Miras

Published online by Cambridge University Press:  12 April 2016

Chris Koen  and
Fred Lombard
Chris Koen
Affiliation:
South African Astronomical Observatory, PO Box 9, Observatory, 7935 Cape, South Africa
Fred Lombard
Affiliation:
Department of Mathematics & Statistics, Rand Afrikaans University, PO Box 524, 2006 Auckland Park, South Africa

Abstract

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A brief rationale for the use of a period test statistic based on the periodogram is given. Results of its application to 380 Mira datasets are summarised.

Type
Part 5. Red Giants, Miras, post-AGB stars and proto-planetary nebulae
Information
International Astronomical Union Colloquium , Volume 193: Variable Stars in the Local Group , 2004 , pp. 357 - 360
Copyright
Copyright © Astronomical Society of the Pacific 2004

References

AAVSO, 1990, Maxima and minima of Long Period Variables. American Association of Variable Star Observers, Cambridge, MA Google Scholar
Koen, C., Lombard, F. 2001, MNRAS, 325, 1124 Google Scholar
Koen, C., Lombard, F. 2004, submittedGoogle Scholar
Lombard, F. 1998, MNRAS, 294, 657 Google Scholar
Lombard, F., Koen, C. 1993, MNRAS, 263, 309 Google Scholar