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V. F. Litvin F. M. Holzmann B. S. Taibin V. S. Popov G. D. Poljakova 《Astronomische Nachrichten》1989,310(1):23-27
Analysing the distribution of the redshift of clusters of galaxies, obtained from the catalogue of SCHMIDT (1986), two already known periodical structures were confirmed and both periods were extended by a number of periods — approximately by two times (We elucidated 5 new periods in the first structure and 4 in the second.). The statistical significance of these structures was estimated to 0.01 in the first case and to 0.02 in the second one. Particularly, the second structure may be the largest known object in the Universe (about 900 Mpc at H = 75 km s-1 Mpc-1). These results agree with the predictions of the axion-dominated early Universe. In addition, we discovered periodical structures of an another type — in luminosity functions of galaxies, which are members of rich clusters. Bei der Analyse des Katalogs von SCHMIDT (1986) wurden zwei periodische Strukturen in den Verteilungen der Rotverschiebungen von Galaxienhaufen festgestellt. In den beiden Strukturen wurden 5 bzw. 4 neue Perioden beobachtet, weshalb sich die Periodenzahl in jeder der beiden Strukturen etwa verdoppelt hat. Die statistische Signifikanzen dieser Strukturen wurden zu 0.01 und 0.02 abgeschätzt. Möglicherweise entspricht die zweite Struktur dem größten bekannten Objekt des Weltalls (etwa 900 Mpc bei H = 75 km s-1 Mpc-1). Diese Resultate stützen die Theorie eines axiondominierten frühen Universums. Außerdem wurden weitere periodische Strukturen in der Leuchtkraftfunktion von Galaxien aus reichen Galaxien-haufen entdeckt. 相似文献
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Christopher Ke-shih Young 《Monthly notices of the Royal Astronomical Society》2004,354(4):1011-1019
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Manuela Magliocchetti Steve J. Maddox Ed Hawkins John A. Peacock Joss Bland-Hawthorn Terry Bridges Russell Cannon Shaun Cole Matthew Colless Chris Collins Warrick Couch Gavin Dalton Roberto de Propris Simon P. Driver George Efstathiou Richard S. Ellis Carlos S. Frenk Karl Glazebrook Carole A. Jackson Bryn Jones Ofer Lahav Ian Lewis Stuart Lumsden Peder Norberg Bruce A. Peterson Will Sutherland Keith Taylor 《Monthly notices of the Royal Astronomical Society》2004,350(4):1485-1494
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Halton Arp 《Journal of Astrophysics and Astronomy》1997,18(4):393-406
Building on evidence starting from 1966, X-ray observations have once again confirmed the association of quasars with low
redshift galaxies. Enough examples of quasar-like objects ejected in opposite directions from nearby, active galaxies have
accumulated so that an empirical evolutionary sequence can be outlined.
The quasars start out with low luminosity and high (z > 2) redshift. As they travel away from their galaxy of origin they
grow in size and decay in redshift. The redshifts drop in steps and near the quantized values of z = 0.6, 0.3, and 0.06 the
quasars become particularly active, ejecting or breaking up into many objects which evolve finally into groups and clusters
of galaxies. The observations massively violate the assumptions of the Big Bang and require continuous, episodic creation
in a non expanding universe of indefinitely large size and age. 相似文献
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