| Abstract | Using archival imaging from the Wide Field Planetary Camera 2 aboard the Hubble Space Telescope, we investigate the stellar populations of the Local Group dwarf spheroidal Andromeda V—a companion satellite galaxy of M31. The color-magnitude diagram extends from above the first ascent red giant branch (RGB) tip to approximately 1 mag below the horizontal branch (HB). The steep well-defined RGB is indicative of a metal-poor system while the HB is populated predominantly redward of the RR Lyrae instability strip. Utilizing Galactic globular cluster fiducial sequences as a reference, we calculate a mean metallicity of [Fe/H] = -2.20 ± 0.15 and a distance of (m - M)0 = 24.57 ± 0.04 after adopting a reddening of E(B - V) = 0.16. This metal abundance places And V squarely in the absolute magnitude-metallicity diagram for dwarf spheroidal galaxies. In addition, if we attribute the entire error-corrected color spread of the RGB stars to an abundance spread, we estimate a range of ~0.5 dex in the metallicities of And V stars. Our analysis of the variable-star population of And V reveals the presence of 28 potential variables. Of these, at least 10 are almost certainly RR Lyrae stars based on their time sequence photometry. Based on observations with the NASA/ESA Hubble Space Telescope, obtained at the Space Telescope Science Institute. |
