Institut d'Astrophysique de Paris, 98bis Boulevard Arago, F-75014 Paris, France;
current affiliation: Kapteyn Laboratorium, Postbus 800, 9700 AV Groningen, The
Netherlands
R. Ferlet
J. B. Marquette
A. Vidal-Madjar
Institut d'Astrophysique de Paris, 98bis Boulevard Arago, F-75014 Paris,
France
Abstract
The EROS project (Experience de Recherche d'Objets Sombres) has
given, as a by-product, numerous and good quality light curves of Cepheid stars in
both the Large Magellanic Cloud (LMC) and Small Magellanic Cloud (SMC). A
catalogue of such objects will be presented, and focus will be made on the particular
aspect of the metallicity effect on the Cepheid distance scale.