Conclusions
Despite the sparsity of data on globular clusters in the Magellanic Clouds and Sculptor-type dwarf galaxies, a preliminary comparison of them with globular clusters of the Galaxy can be made.
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1)
If observational selection does not seriously distort the results, there is a higher fraction of young globular clusters among those in the Magellanic Clouds that have a horizontal branch than among the globular clusters of the Galaxy. In addition, the clusters in Lhe Large Cloud are older than those in the Small Cloud.
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2)
To the know similarities between globular clusters and Sculptor-type dwarf elliptic galaxies one can add the following characteristics of the latter: a) the α distribution, b) the values of r, and c) position on the α-r diagram. If these parametess reflect the history of development of the corresponding systems, this similarity suggests that the observed stage of stellar evolution is similar in Sculpto r-type globular clusters.
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Additional information
Astronomical Observatory, L'vov University. Translated from Astrofizika, Vol. 9, No. 4, pp. 589–593, October–December, 1973.
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Éigenson, A.M. Horizontal branch in globular clusters of the galaxy and the magellanic clouds in sculptor-type dwarf galaxies. Astrophysics 9, 356–358 (1973). https://doi.org/10.1007/BF01002521
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DOI: https://doi.org/10.1007/BF01002521