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.
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References
Dapergolas, A., Kontizas, E. and Kontizas, M.: 1986, Astron. Astrophys. Suppl. Ser., 65, 283.
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Kontizas, E., Kontizas, M., Dapergolas, A. and Hadzidimitriou, D.: 1987b IAU Symp. No. 126. (in press).
Westerlund, B.: 1961, Uppsala Astronomiska Observatoriums Annaler, Bond 5, No. 2, p. 3.
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© 1989 Kluwer Academic Publisher
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Dapergolas, A., Kontizas, E., Kontizas, M., Pasian, F., Pucillo, M., Santin, P. (1989). An Age Estimate for the NGC456, 460 and 465 SMC Constellation. In: Caffo, M., Fanti, R., Giacomelli, G., Renzini, A. (eds) Astronomy, Cosmology and Fundamental Physics. Astrophysics and Space Science Library, vol 155. Springer, Dordrecht. https://doi.org/10.1007/978-94-009-0965-6_34
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DOI: https://doi.org/10.1007/978-94-009-0965-6_34
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