Abstract
Chains ofnormal galaxies dominate small-scale clustering. This filamentary structure has nothing to do with large-scale filaments between clusters; and the revelation of short galaxy chains among normal galaxies was not expected by Arp, who investigated chains ofpeculiar galaxies. The nature of revealed chains cannot be explained in terms of so-called filaments observed in a scale of 100 Mpc: there is no continuation between 100 kpc and 100 Mpc chains of galaxies.
Three sorts of clustering modes, corresponding toG 1,G 2 andG 4 non-isomorphic graphs withthree vertices, are free of the time paradox. Chains (the clustering mode corresponding to theG 3 graph) are stable on a time scale less (tens and sometimes a hundred times) than the conventional age ofnormal galaxies. Why do the chains dominate small scales?
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References
Bereś, H.: 1987a, in:The Algorithms of Selected Problems in a Cluster Analysis, Kielce Tech. Univ. Press, Kielce, Extragalactic Astronomy Programme, 21.
Bereś, K.: 1987b,ibid., 43.
Bereś, K.: 1987c,ibid., 51.
Einasto, M.,et al.: 1989,Monthly Notices of the RAS 238, 155.
Garncarek, Z.: 1980, Ph.D. Thesis, Jagellonian University.
Garncarek, Z.: 1986,Acta Cosmologica 14, 101.
Garncarek, Z.: 1987a, in:The Algorithms of Selected Problems in a Cluster Analysis, Kielce Tech. Univ. Press, Kielce, Extragalactic Astronomy Programme, 9.
Garncarek, Z.: 1987b,ibid., 13.
Garncarek, Z.: 1989,Acta Cosmologica 16, 37.
Garncarek, Z. and Rudnicki, K.: 1990,Apeiron 8, 16.
Grabińska, T.: 1983, Celebration of the Centenary (1882–1982) of the Birth of Thaddeus Banachiewicz,Development of Techniques of Astronomical and Geodetic Calculations, Kraków, 20–21 May, (“The Self-Similarity Technique and Fractal Distribution of Mass in Astronomical Aggregates”, Scientific Bulletins of Stanisław Staszic Academy at Kraków, Geodesy - Bulletin 87 - Geodezja1000, 84 (1986), vol. II; Vol. I of the 100th Birthday Anniversary of Thaddeus Banachiewicz published in Geodesy - Bulletin 86 - Geodezja999 (1986), Jan Mietelskiet al. (eds.), PL ISSN 0452-6457).(“The jubilee could not be celebrated in 1982 because of some obstacles” (from the Preface of Prof. M. Odlanicki-Poczobutt, p.9.; i.e., the anti-Solidarity state-of-war which blocked the liberation of a part of Europe; and the honorary guest, Prof. Z. Kopal, was unable to join the conference “Development of Techniques ...”.
Grabińska, T.: 1985,Astrophys. Space Sci. 115, 369.
Grabińska, T.: 1986,The Hierarchical Structure of the Universe, in: “COSMOS-an Educational Challenge”, ESA-SP 253, European Space Agency, Paris, p. 303.
Grabińska, T.: 1988,Astrophys. Space Sci. 150, 75.
Grabińska, T.: 1989a,Astrophys. Space Sci. 161, 347.
Grabińska, T.: 1989b, “The Further Search of Voids in the Jagellonian Field”, in:From Stars to Quasars: Devoted to Prof. Wilhelmina Iwanowska, S. Grudzińska and B. Krygier (eds.), University of Mikołaj Kopernik at Toruń, Astronomical Observatory, Toruń, 125.
Iwanowska, W.: 1989, “The Local Group of Galaxies”, in:From Stars to Quasars: Devoted to Prof. Wilhelmina Iwanowska, S. Grudzińska and B. Krygier (eds.), University of Mikołaj Kopernik at Toruń, Astronomical Observatory, Toruń 55.
Lachièze-Rey, M.: 1986, “Fractals and Galaxy Distribution”, Preprint IRF-SAp CEN Saclay, 1-13.
McNally, D.: 1986, “The Birth of Stars”, in:COSMOS - An Educational Challenge, European Space Agency, No. ESA SP-253, Paris, 51.
Rudnicki, K.: 1978, “Methods of the Investigation of the Distribution of Points”, in:The Algorithms of Selected Problems in a Cluster Analysis, Zeszyty Naukowe Politechniki Swietokrzyskiej, Problemy Nauk Podstawowych No. 17, Technical University at Kielce, Extragalactic Astronomy Programme (K. Bereś and H. Bereś), PL ISSN 0860-2077, Kielce, 5.
Rudnicki, K. and Danielkiewicz-Krośniak, E.: 1989,Acta Cosmol. 16, 45.
Rudnicki, K.et al.: 1973,Acta Cosmologica 1, 7.
Rudnicki, K.et al.: 1985,Nuovo Cimento 8C, 368.
Rudnicki, K.et al.: 1989a,Comments on Astroph. 13, 171.
Rudnicki, K.et al.: 1989b, “Intergalactic Dust and the Various Schemes of Evolution of the Universe”, in:From Stars to Quasars: Devoted to Prof. Wilhelmina Iwanowska, S. Grudzińska and B. Krygier (eds.), University of Mikołaj Kopernik at Toruń, Astronomical Observatory, Toruń, 119.
Tarraro, I.: 1974,Postepy Astronomii 22, 345.
Tarraro, I.: 1977,Acta Cosmologica 6, 55.
Seitter, W.C.,et al.: 1989, “Problems and Solutions in Observational Cosmology”, in:Morphological Cosmology, Proceed. XIth Cracow Cosmological School, held in Cracow, August 22–31, 1988, P. Flin and H. W. Duerbeck (eds.), (Lecture Notes in Physics 322), Springer Verlag, Berlin, p. 3
Wszołek, B.: 1989, “Dusty Intergalactic Matter”, in:ibid., 178.
Wszołek, B.: 1988, Postepy Astronomii36, 245.
Zieba, A.: 1975,Acta Cosmol. 3, 75.
Zieba, S.: 1977, Hab. Thesis, Jagiellonian University.
Zieba, S.: 1988,Acta Cosmologica 15, 85.
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Zabierowski, M. The G3 non-isomorphic clustering graph and the problem of the physical reality of the clustering tendency. Astrophys Space Sci 201, 125–130 (1993). https://doi.org/10.1007/BF00626981
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DOI: https://doi.org/10.1007/BF00626981