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AGB variables as distance indicators

Published online by Cambridge University Press:  12 April 2016

Michael Feast*
Affiliation:
Astronomy Department, University of Cape Town, Rondebosch 7701, South Africa

Abstract

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Evidence for the existence of Mira Period-Luminosity relations is reviewed including recent work on Miras with thick circumstellar shells. The calibration of the relation at K is discussed in detail. The nature of variables deviating from the PL relation and possible metallicity effects are also discussed.

Type
Part 5. Red Giants, Miras, post-AGB stars and proto-planetary nebulae
Copyright
Copyright © Astronomical Society of the Pacific 2004

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