An Age Estimate for the NGC456, 460 and 465 SMC Constellation

  • A. Dapergolas
  • E. Kontizas
  • M. Kontizas
  • F. Pasian
  • M. Pucillo
  • P. Santin
Conference paper
Part of the Astrophysics and Space Science Library book series (ASSL, volume 155)

Abstract

The aim of this paper is to study the distribution of spectral types of the stellar content in an outlying region (wing) of the Small Magellanic Cloud (SMC) which contains the brightest early type stars and therefore the most massive in this galaxy.

Keywords

Spectral Type Type Star Late Type Star Spectral Classification Small Magellanic Cloud 
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.

References

  1. Dapergolas, A., Kontizas, E. and Kontizas, M.: 1986, Astron. Astrophys. Suppl. Ser., 65, 283.ADSGoogle Scholar
  2. Kontizas, E., Morgan, D.H., Dapergolas, A. and Kontizas, M.: 1987a, Astron. Astrophys. Suppl. Ser., 70, 1.ADSGoogle Scholar
  3. Kontizas, E., Kontizas, M., Dapergolas, A. and Hadzidimitriou, D.: 1987b IAU Symp. No. 126. (in press).Google Scholar
  4. Westerlund, B.: 1961, Uppsala Astronomiska Observatoriums Annaler, Bond 5, No. 2, p. 3. Google Scholar

Copyright information

© Kluwer Academic Publisher 1989

Authors and Affiliations

  • A. Dapergolas
    • 1
  • E. Kontizas
    • 1
  • M. Kontizas
    • 2
  • F. Pasian
    • 3
  • M. Pucillo
    • 3
  • P. Santin
    • 3
  1. 1.Astronomical InstituteNational Observatory of AthensGR-AthensGreece
  2. 2.University of AthensAthensGreece
  3. 3.Osservatorio Astronomico di TriesteTriesteItaly

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