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RR Lyrae Stars and the Sandage Period-Shift Effect Examined Using IR-Derived Temperatures

Published online by Cambridge University Press:  12 April 2016

A.J. Longmore
Affiliation:
Royal Observatory, Edinburgh
R. Dixon
Affiliation:
University of Edinburgh
I. Skillen
Affiliation:
University of Leicester
R.F. Jameson
Affiliation:
University of Leicester
J.A. Fernley
Affiliation:
University College, London

Abstract

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Mean temperatures for RR Lyrae stars in 7 globular clusters (M3, M4, M5, M15, M107, ω Cen and NGC 5466) have been determined using the optical-infrared colour <V>-<K> as a temperature indicator. Where <K> has been relatively well determined, from means of 3 or more observations, the scatter in relationships such as Log P’ vs log (temperature) and log (temperature) vs (blue amplitude) is significantly reduced when IR-derived temperatures are used instead of those derived from (B-V). Within the observational errors, the gradient in the log P’ vs log (temperature) diagram is the same for each cluster. Temperatures derived from <V>-<K> should also be less sensitive to metallicity differences than their optically derived counterparts. The Sandage Period-Shift Effect has therefore been re-examined using 6 of the 7 clusters (NGC 5466 was excluded because of too few data). A strong correlation between period-shift and metallicity is found; a smaller shift (but in the same sense) is also found for the temperature – amplitude relationship.

Type
4. Abstracts of Poster Papers
Copyright
Copyright © Cambridge University Press 1989