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Stellar Populations in M31 and M33

Published online by Cambridge University Press:  07 August 2017

S. Van Den Bergh  and
C.J. Pritchet
S. Van Den Bergh
Affiliation:
Dominion Astrophysical Observatory National Research Council 5071 West Saanich Road Victoria, B.C., V8X 4M6, Canada
C.J. Pritchet
Affiliation:
Department of Physics and Astronomy University of Victoria Box 3055 Victoria, B.C., V8W 3P6, Canada

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M31 and M33 are the two nearest extragalactic spirals. They are therefore particularly suitable for studies of stellar populations. From integrated photometry spiral galaxies are known to consist of four components: (1) a nucleus, (2) a nuclear bulge, (3) an (exponential) disk and (4) a halo. These stellar components are embedded within a massive invisible halo.

Type
II. The Stellar Populations of Nearby Resolved Galaxies
Information
Symposium - International Astronomical Union , Volume 149: The Stellar populations of Galaxies , 1992 , pp. 161 - 168
Copyright
Copyright © Kluwer 

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