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Star Counts in Fields Surrounding the LMC

Published online by Cambridge University Press:  04 August 2017

M.T. Brück
M.T. Brück*
Affiliation:
Department of Astronomy, University of Edinburgh, Royal Observatory, Edinburgh EH9 3HJ

Abstract

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Star counts in a number of fields near the Large Magellanic Cloud have shown a maximum extension of about 10° for the faint stars. The luminosity function in the outer regions of the LMC is consistent with an intermediate age population.

Type
Evolution
Information
Symposium - International Astronomical Union , Volume 108: Structure and Evolution of the Magellanic Clouds , 1984 , pp. 97 - 98
Copyright
Copyright © Reidel 1984 

References

Brück, M.T.: 1978, Astron. Astrophys. 68, 181 Google Scholar
Brück, M.T.: 1980, Astron. Astrophys. 87, 92 Google Scholar
Butcher, H.: 1977, Astrophys. J. 216, 372 Google Scholar
Butler, C.J.: 1976, Dunsink Obs. Publ. 1, No.6 Google Scholar
Kunkel, W.: 1980, IAU Symp. 85 (ed. Hesser, J.E.) p. 353 Google Scholar
Martin, W.L.: 1977, Mem. Roy. ast. Soc. 83, 69 Google Scholar
Stryker, L. and Butcher, H.: 1982, IAU Colloq. 68 (ed. Davis Philip, A.G. and Hayes, D.S.) p. 255 Google Scholar