Variable Stars in Metal-Rich Globular Clusters. IV. Long Period
  Variables in NGC 6496
  We present VI-band photometry for stars in the metal-rich globular cluster
NGC 6496. Our time-series data were cadenced to search for long period
variables (LPVs) over a span of nearly two years, and our variability search
yielded the discovery of thirteen new variable stars, of which six are LPVs,
two are suspected LPVs, and five are short period eclipsing binaries. An
additional star was found in the ASAS database, and we clarify its type and
period. We argue that all of the eclipsing binaries are field stars, while 5-6
of the LPVs are members of NGC 6496. We compare the period-luminosity
distribution of these LPVs with those of LPVs in the Large Magellanic Cloud and
47 Tucanae, and with theoretical pulsation models. We also present a VI color
magnitude diagram, display the evolutionary states of the variables, and match
isochrones to determine a reddening of E(B-V) ~ 0.21 mag and apparent distance
modulus of ~ 15.60 mag.
