The Nuclear Regions of M31, M32, and M33 Imaged by HST

  • R. M. Rich
  • K. J. Mighell
  • J. D. Neill
  • W. L. Freedman
Conference paper
Part of the Astrophysics and Space Science Library book series (ASSL, volume 209)

Abstract

The nearest massive members of the Local Group- M31, M32, and M33- give us a window on the stellar populations and dust in the central 100 pc of galaxies. We report new imaging of the stellar populations and dust in the central 100 pc of these galaxies using HST and WFPC2.

Keywords

Globular Cluster Nuclear Region Stellar Population Bright Star Color Plate 
These keywords were added by machine and not by the authors. This process is experimental and the keywords may be updated as the learning algorithm improves.

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Copyright information

© Kluwer Academic Publishers 1996

Authors and Affiliations

  • R. M. Rich
    • 1
  • K. J. Mighell
    • 1
  • J. D. Neill
    • 1
  • W. L. Freedman
    • 2
  1. 1.Columbia UniversityNYUSA
  2. 2.Observatories of the Carnegie Instiution of WashingtonPasadenaUSA

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