Summary
It is necessary to examine the significance of the recently discovered peak of spatial two-point correlation function determined for the rich Abel clusters. We discuss the different possibilities to do it and propose the programme of further observations.
Riassunto
È necessario esaminare il significato del picco recentemente scoperto della funzione di correlazione a due punti spaziale determinata per i cluster ricchi di Abell. Si discutono le diverse possibilità di farlo e si propone la programmazione di ulteriori osservazioni.
Резюме
Отмечается важность исследования недавно обнаруженного пика пространственной функции двух-точечной корреляции, определенной для больших Абеллевых кластеров. Мы обсуждаем различные возможности проведения исследований и предлагаем программу дальнейших наблюдений.
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References
V. F. Shvartsman:Heads of a Report on the Fifth All-Union Conference on Gravitation and Relativity (Moscow, 1981), p. 219.
A. I. Kopylov, T. S. Fetisova andV. F. Shvartsman:Astron. Tsirk.,1344, 1 (1984).
A. I. Kopylov, D. Yu. Kuznetsov, T. S. Fetisova andV. F. Shvartsman:Astron. Tsirk.,1347, 1 (1984).
A. I. Kopylov, V. A. Lipovetskji, T. S. Fetisova andV. F. Shvartsman:Astron. Tsirk.,1393, 1 (1984).
A. I. Kopylov, D. Yu. Kuznetsov, T. S. Fetisova andV. F. Shvartsman:Special Astrophys. Obs. Commun.,53, 39 (1987).
G. O. Abell:Astrophys. J., Suppl. Ser.,3, 211 (1958).
F. Zwicky, E. Herzog, P. Wild, M. Karpowicz andS. T. Kowai:Catalogue of Galaxies and Clusters of Galacies (Cal. Inst. of Tech., D. Pasadena, Cal. 1961–1968).
N. A. Bahcall andR. M. Soneira:Astrophys. J.,270, 20 (1983).
A. A. Klypin andA. I. Kopylov:Pis’ma Astron. Ž.,9, 75 (1983).
D. Yu. Kuznetsov andV. A. Lipovetskij:Special Astrophys. Obs. Commun.,53, 92 (1987).
D. D. Sokolov andV. F. Shvartsman:Ž. Ėksp. Teor. Fiz.,66, 412 (1974).
N. S. Kardashev, H. J. Blome andW. Priester: Preprint of Space Research Inst., A. S. USSR, No. 1259 (1987).
A. A. Leir andS. van den Bergh:Astrophys. J., Suppl. Ser.,34, 381 (1977).
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Kuznetsov, D.Y., Fetisova, T.S. Arguments in favour of physical reality of the peculiar (200÷300) Mpc scale in the distribution of the rich clusters of galaxies. Il Nuovo Cimento C 12, 639–647 (1989). https://doi.org/10.1007/BF02508021
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DOI: https://doi.org/10.1007/BF02508021