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M. Zabierowski 《Astrophysics and Space Science》1988,141(2):333-338
The property of anthropomorphism as it is held in fractal cosmography is reconstructed.Man is only interested in the probability distribution of mass in cases where mass does not vanish, and he finds no help at all to be told that such cases almost never occur. 相似文献
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We discuss Arp's hypothesis that the HII regions are more numerous and more conspicuous on the side of a galaxy facing its companion. Arp's hypothesis seems not to be true if we add to Hodge's sets of galaxies only the most probably tidally-interacting cases. 相似文献
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The possibility of the variation of the gravitational constant with space coordinates is considered.Published in Astrofizika, Vol. 37, No. 2, pp. 363–366, April–June, 1994. 相似文献
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M. Zabierowski 《Astrophysics and Space Science》1993,202(1):173-178
The perspective given by Iwanowska (inFrom Stars to Quasars, Toru, 1989, volume devoted to Prof. Iwanowska) is developed. The redshifts of the Iwanowska's lines galaxies form five states. We used all the redshifts indicated in the Iwanowska's concept. Our hypotheses can be easily verified in the future checking the new redshifts of galaxies belonging to five lines of galaxies selected by Iwanowska. This solution of the problem of stability of the lines is in serious disagreement with the concept of an anthropic universe advocated by Barrow, Tipler, and Wheeler, nevertheless it fits the view of Grabiska on the problem of antropicity, observation, evaluation of extragalactic data and meta-astronomy, cf. T. GrabiskaRealism and Instrumentalism in Contemporary Physics, Wroclaw Technological Institute, 1992, M. Zabierowski,Status of the Observer in Contemporary Physics, Institute of Physics, 1990. 相似文献
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Published in Astrofizika, Vol. 37, No. 2, pp. 307–312, April–June, 1994. 相似文献
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Miroslaw Zabierowski 《Astrophysics and Space Science》1985,111(1):179-188
Based on diurnal values of the total radio-flux density at 10.7 cm as well as on corresponding Zürich numbers the relation giving the radio-flux as function ofR is established. The behaviour of low and high values ofR andF
2800 during the time interval 1957–1976 is studied. Preliminary conclusions drawn by other investigators are confirmed. A prediction of the total radio-flux for the 22nd solar cycle is given. 相似文献
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M. Zabierowski 《Astrophysics and Space Science》1993,201(1):125-130
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? 相似文献
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The use of a cosmic potential in relativistic cosmology is criticized. It is pointed out that the energetic closure of the Universe follows from general relativity and from quantized superspace cosmology without the introduction of the cosmic potential. 相似文献
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M. Zabierowski 《Astrophysics and Space Science》1981,74(2):487-489
Additional evidence is put forward, bearing on Melik-Alaverdian's paper On the Problem of the Distribution of O-B Stars, in which he concluded that the observed distribution of stars contradicts the standard approach to star formation. 相似文献
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