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Paper: Isolating Red Giants in M31's Outer Spheroid: The Metallicity Gradient
Volume: 92, Formation of the Galactic Halo. . . . Inside and Out
Page: 540
Authors: Reitzel, David B.; Guhathakurta, Puragra; Gould, Andrew
Abstract: The aim of our project is to measure the metallicity gradient in the spheroid of the Andromeda galaxy (M31). Deep KPNO 4-m UBRI images of a 15'times15 ' field in the outer spheroid of M31 are being used to isolate a sample of red giant branch (RGB) stars. These stars are distinguished from the more numerous distant field galaxies on the basis of broadband colors and image morphology. This technique yields a sample of candidate RGBs in M31's spheroid, located about 20kpc from its center (in projection). The shape of the M31 RGB is compared to those of Galactic globular clusters spanning a wide range of (known) metallicities.
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