Variable stars in the unusual, metal-rich, globular cluster NGC 6441

We have undertaken a search for variable stars in the metal-rich globular c luster NGC 6441 using time-series BV photometry. The total number of variab les found near NGC 6441 has been increased to similar to 104, with 48 new v ariables being found in this survey. A significant number of the variables are RR Lyrae stars (similar to 46), most of which are probable cluster memb ers. As was noted by Layden et al. in 1999, the periods of the fundamental- mode RR Lyrae stars are unusually long compared with field stars of similar metallicity. The existence of these long-period RRab stars is consistent w ith Sweigart & Catelan's prediction that the horizontal branch of NGC 6441 is unusually bright. This result implies that the metallicity-luminosity re lationship for RR Lyrae stars is not universal. We discuss the difficulty i n determining the Oosterhoff classification of NGC 6441 because of the unus ual nature of its RR Lyrae stars. A number of ab-type RR Lyrae stars are fo und to be both brighter and redder than the other probable RRab found along the horizontal branch, which may be a result of blending with stars of red der color. A smaller than usual gap is found between the shortest period fu ndamental-mode and the longest period first-overtone-mode RR Lyrae stars. W e determine the reddening of the cluster to be E(B-V) = 0.51 +/- 0.02 mag, with substantial differential reddening across the face of the cluster. The mean V magnitude of the RR Lyrae is found to be 17.51 +/- 0.02 mag, result ing in a distance of 10.4-11.9 kpc, for a range of assumed values of [M-V] for RR Lyrae stars. The possibility that stars in NGC 6441 may span a range in [Fe/H] is also discussed.