Abstract
In star clusters and in galaxy clusters the exponentn of the generalized law of Schuster statistically decreases with increasing masses\(\mathfrak{M}\) of the clusters or increasing numbersL of their members. In most casesn(gal. cl.) is smaller thann(st. cl.). It is confirmed, that in larger galaxy clusters the brighter members are somewhat more concentrated at the center than the fainter members.
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Literatur
Bahcall, N. A.: 1971,Astrophys. J. 76, 995.
Bahcall, N. A.: 1972,Astron. J. 77, 550.
Baier, F. W.: 1977,Astron. Nachr. 298, 151.
Baier, F. W.: 1979,Astron. Nachr. 300, 133.
Baier, F. W. und Mai, M.: 1978,Astron. Nachr. 299, 69.
Kwast, T.: 1966,Acta Astron. 16, 45.
Lohmann, W.: 1964,Z. Astrophys. 60, 43.
Lohmann, W.: 1971,Astron. Nachr. 292, 193;Mitt. Astron. Rechen-Inst. Heidelberg (B), Nr. 29.
Lohmann, W.: 1972,Astron. Nachr. 293, 259;Mitt. ARI (B), Nr. 30.
Lohmann, W.: 1975,Astrophys. Space Sci. 32, 153;Mitt. ARI (A), Nr. 88.
Miczaika, G. R.: 1947,Veröff. Landessternw. Heidelberg 14, Nr. 15.
Noonan, T. W.: 1972,Astron. J. 77, 9.
Rudnicki, R.: 1963,Acta Astron. 13, 230.
Zwicky, F.: 1937,Astrophys. J. 86, 217.
Zwicky, F.: 1950,Publ. Astron. Soc. Pacific 62, 196.
Zwicky, F.: 1951,Publ. Astron. Soc. Pacific 63, 61.
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Lohmann, W. Über Den Aufbau Der Stern- Und Galaxienhaufen. Astrophys Space Sci 72, 439–446 (1980). https://doi.org/10.1007/BF00639149
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DOI: https://doi.org/10.1007/BF00639149