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The Stellar Populations in the Disk of M31
Published online by Cambridge University Press: 07 August 2017
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CCD observations have been carried on 4 fields in the outer disk and one in the halo of M31 on the 5m Hale telescope, and reduced using the Starman stellar photometry package (Penny, 1992). CMDs for all fields show the brightest 3 magnitudes of the Red Giant Branch. AGB luminosity functions were constructed for each field and corrected for incompletness. Full details are given in Morris et al (1994).
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- Copyright © Kluwer 1995