Abstract
A computational model is developed for the origin of protogalactic eddies at the fronts of large-scale ‘pancake’ shocks. Possible effects of orientation of spiral galaxies in their pairs, groups, clusters and superclusters are discussed.
References
Chernin, A. D.: 1970,Nature 226, 440.
Chernin, A. D. and Zentsova, A. S.: 1980,Astron. Astrophys. 89, 1.
Chernin, A. D., Silbergleit, A. S., and Tropp, E. A.: 1976,Astrophys. Space Sci. 43, 175.
Doroshkevich, A. G.: 1973,Astrophys. Letters 14, 11.
Hoyle, F.: 1951, inProblems of Cosmic Aerodynamics, Dayton, Ohio, p. 195.
Kapranidis, S. and Sullivan, W. T., III: 1983,Astrophysics 118, 33.
Karachentsev, I. D.: 1981,Astrofizika 17, 675, 693.
Kontorovich, V. M.: 1957,J. Exp. Theoret. Phys. 33, 1527.
McKenzie, J. F. and Westphal, K. O.: 1970,Phys. Fluids 13, 630.
Ostriker, J. and Cowie, L.: 1981,Astrophys. J. 243, L127.
Peebles, P. J. E.: 1969,Astrophys. J. 155, 393.
Peebles, P. J. E.: 1971,Astrophys. Space Sci. 11, 443.
Sunyaev, R. A. and Zeldovich, Ya. B.: 1972,Astron. Astrophys. 20, 189.
Vorontsov-Velyaminov, B. A.: 1978,Extragalactic Astronomy, Nauka, Moscow.
Zeldovich, Ya. B.: 1970,Astron. Astrophys. 5, 84.
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Chernin, A.D., Ushakov, A.Y. Angular momentum of galaxies and the structure of protogalactic vorticity. Astrophys Space Sci 96, 217–221 (1983). https://doi.org/10.1007/BF00661956
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DOI: https://doi.org/10.1007/BF00661956