A&A 429, L37-L40 (2005)
DOI: 10.1051/0004-6361:200400110
Letter
The influence of chemical composition on the properties of Cepheid stars
I. Period-Luminosity relation vs. iron abundance
M. Romaniello1, F. Primas1, M. Mottini1, M. Groenewegen2, G. Bono3 and P. François41 European Southern Observatory, Karl-Schwarzschild-Strasse 2, 85748 Garching bei München, Germany
e-mail: mromanie@eso.org
2 Instituut voor Sterrenkunde, PACS - ICC, Celestijnenlaan 200B, 3001 Leuven, Belgium
3 INAF - Osservatorio Astronomico di Roma, via di Frascati 33, 00040 Monte Porzio Catone, Italy
4 Observatoire de Paris-Meudon, GEPI, 61 avenue de l'Observatoire, 75014 Paris, France
(Received 11 October 2004 / Accepted 20 November 2004)
Abstract
We have assessed the influence of the stellar iron content on the
Cepheid Period-Luminosity (
PL) relation by relating the
V band
residuals from the Freedman et al. (2001)
PL relation to
[Fe/H] for 37 Galactic and Magellanic Clouds Cepheids. The iron
abundances were measured from FEROS and UVES high-resolution and
high-signal to noise optical spectra. Our data indicate that the stars
become fainter as metallicity increases, until a plateau or turnover
point is reached at about solar metallicity. Our data are incompatible
with both no dependence of the
PL relation on iron abundance, and
with the linearly decreasing behavior often found in the literature
(e.g. Kennicutt et al. 1998; Sakai et al. 2004). On the
other hand, non-linear theoretical models of Fiorentino et
al. (2002) provide a fairly good description of the data.
Key words: stars: abundances -- stars: distances -- Cepheids
SIMBAD Objects
© ESO 2004

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