To appear in The Astronomical Journal

  • T. J. Davidge
  • Published 1994

Abstract

Deep V and I CCD images with sub-arcsec spatial resolution are used to investigate the stellar content of the central regions of the Local Group dwarf elliptical galaxy NGC147. Red giant branch (RGB) stars are resolved over the entire field, and the RGB-tip occurs at I ∼ 20.5, suggesting that the distance modulus is 24.3. A comparison with globular cluster… (More)

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