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The Stellar Populations in the Disk of M31

Published online by Cambridge University Press:  07 August 2017

P.W. Morris ,
W. Griffiths ,
I.N. Reid ,
A.J. Penny  and
R.J. Dickens
P.W. Morris
Affiliation:
Department of Physics, Leeds University, Leeds, UK; Caltech, USA; Rutherford Appleton Laboratory, UK
W. Griffiths
Affiliation:
Department of Physics, Leeds University, Leeds, UK; Caltech, USA; Rutherford Appleton Laboratory, UK
I.N. Reid
Affiliation:
Department of Physics, Leeds University, Leeds, UK; Caltech, USA; Rutherford Appleton Laboratory, UK
A.J. Penny
Affiliation:
Department of Physics, Leeds University, Leeds, UK; Caltech, USA; Rutherford Appleton Laboratory, UK
R.J. Dickens
Affiliation:
Department of Physics, Leeds University, Leeds, UK; Caltech, USA; Rutherford Appleton Laboratory, UK

Extract

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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).

Type
Poster Papers
Information
Symposium - International Astronomical Union , Volume 164: Stellar Populations , 1995 , pp. 412
Copyright
Copyright © Kluwer 1995 

References

Innanen, K.A., Kamper, K.W., Papp, K.A., and van den Bergh, S., 1982, ApJ, 254, 515 CrossRefGoogle Scholar
Morris, P.W., Reid, I.N., Griffiths, W.K., and Penny, A.J., 1994, MNRAS, accepted Google Scholar
Penny, A.J., Starman A stellar photometry/Image and Table handling package, Starlink Project, Starlink User Note 141.1 Google Scholar