Baade-Wesselink distances and the effect of metallicity in classical cepheids
Koninklijke Sterrenwacht van België, Ringlaan 3, 1180 Brussels, Belgium e-mail: email@example.com
2 Instituut voor Sterrenkunde, Celestijnenlaan 200 D, 3001 Leuven, Belgium
Accepted: 3 June 2008
Context. The metallicity dependence of the Cepheid PL-relation is of importance in establishing the extra-galactic distance scale.
Aims. The aim of this paper is to investigate the metallicity dependence of the PL-relation in V and K based on a sample of 68 Galactic Cepheids with individual Baade-Wesselink distances (some of the stars also have an HST-based parallax) and individually determined metallicities from high-resolution spectroscopy.
Methods. Literature values of the V-band, K-band and radial velocity data have been collected for a sample of 68 classical cepheids that have their metallicity determined in the literature from high-resolution spectroscopy. Based on a surface-brightness relation and a projection factor derived in a previous paper, distances have been derived from a Baade-Wesselink analysis. PL- and PLZ-relations in V and K are derived.
Results. The effect of the adopted dependence of the projection factor on period is investigated. The change from a constant p-factor to one recently suggested in the literature with a mild dependence on results in a less steep slope by 0.1 unit, which is about the 1-sigma error bar in the slope itself. The observed slope in the PL-relation in V in the LMC agrees with both hypotheses. In K the difference between the Galactic and LMC slope is larger and would favour a mild period dependence of the p-factor. The dependence on metallicity in V and K is found to be marginal, and independent of the choice of p-factor on period. This result is severely limited by the small range in metallicity covered by the Galactic Cepheids.
Key words: stars: distances / stars: variables: cepheids / cosmology: distance scale / stars: oscillations including pulsations
© ESO, 2008