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The slope of the RR Lyrae MV–[Fe/H] relation
Authors:Fernley,Carney,Skillen,Cacciari,&   Janes
Affiliation:IUE Observatory, Apdo 50727, 28080 Madrid, Spain,;Department of Physics and Astronomy, University of North Carolina, Chapel Hill, NC 27599, USA,;STScI, 3700 San Martin Drive, Baltimore, MD 21218, USA,;Department of Astronomy, Boston University, 725 Commonwealth Avenue, Boston, MA 02215, USA
Abstract:We review the available observational data to show that the slope of the RR Lyrae MV –[Fe/H] relation is 0.18±0.03. The recent claim by Feast that, because of biases, the true slope is much steeper is not justified.
Keywords:stars: variables: other    globular clusters: general.
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