Light curves and metal abundances of RR Lyrae variables in the bar of the Large Magellanic Cloud

Details Light curves and metal abundances of RR Lyrae variables in the bar of the Large Magellanic Cloud Light curves and metal abundances of RR Lyrae variables in the bar of the Large Magellanic Cloud

1999-09-20

arxiv.org/abs/astro-ph/9909332v1

Astronomy and Astrophysics

Astrophysics

4 pages including 2 postscript figures, LaTex using newpasp.sty (included). Proceedings of the IAU176 Colloquium, Budapest, Hu

Scientific paper

The Large Magellanic Cloud (LMC) is widely considered a corner-stone of the astronomical distance scale, however a difference of 0.2-0.3 mag exists in its distance as predicted by the "short" and "long" distance scales. Distances to the LMC from Population II objects are founded on the RR Lyrae variables. We have undertaken an observational campaign devoted to the definition of the average apparent luminosity and to the study of the mass-metallicity relation for RR Lyraes in the bar of the LMC. These are compared with analogous quantities for cluster RR Lyraes. The purpose is to see whether an intrinsic difference in luminosity, possibly due to a difference in mass, might exist between field and cluster RR Lyraes, which could be responsible for the well-known dichotomy between "short" and "long" distance scales. Preliminary results are presented on the V and B-V light curves, the average apparent visual magnitude, and the pulsational properties of 102 RR Lyrae in the bar of the LMC, observed at ESO in January 1999. The photometric data are accurately tied to the Johnson photometric system. Comparison is presented with the photometry of RR Lyraes in the bar of the LMC obtained by the MACHO collaboration (Alcock et al. 1996). Our sample includes 9 double-mode RR Lyraes selected from Alcock et al. (1997) for which an estimate of the metal abundance from the DeltaS method is presented.

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