By J. H. Oort (auth.), F. Mardirossian, G. Giuricin, M. Mezzetti (eds.)
The large-scale constitution of the Universe and platforms Clusters, and teams of galaxies are subject matters like Superclusters, They absolutely justify the assembly on "Clusters of serious curiosity. and teams of Galaxies". the themes coated incorporated the spatial distribution and the clustering of galaxies; the houses of Superclusters, Clusters and teams of galaxies; radio and X-ray observations; the matter of unseen topic; theories referring to hierarchical clustering, pancakes, cluster and galaxy formation and evolution. The assembly was once held on the overseas middle for Theoretical Physics in Trieste (Italy) from September thirteen to September sixteen, 1983. It used to be attended via approximately a hundred and fifty contributors from 22 countries who provided sixty seven invited lectures (il) and contributed papers (cp), and forty five poster papers (pp). The clinical Organizing Committee consisted of F. Bertola, P. Biermann, A. Cavaliere, N. Dallaporta, D. Gerba1, M. Hack, J . V . Peach, D. Sciama (Chairman), G. Setti, M. Tarenghi. we're quite indebted to D. Sciama, A. Cavaliere and F. Bertola for his or her paintings of coordination. We have been appearing because the 3 contributors of the neighborhood Organizing Committee. in addition, we're happy to thank the Chairmen of the classes (M. Hack, N. Da11aporta, G. Burbidge, B. turbines, M. Rees, P. Biermann, L.Z. Fang, L. Gouguenheim) for his or her worthwhile help.
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Extra info for Clusters and Groups of Galaxies: International Meeting Held in Trieste Italy, September 13–16, 1983
No. 63. C. 1976, A6btophy,6. J. 203, 23. , and de Vaucouleurs, G. 1980, A6btophy,6. J. Lett. 242, L 153. , and de Vaucouleurs, G. 1983, A6bton. A6btophY-6. 118, 4. -Th. 1983, Mitt. A6bton. GueLe 58, in press. , and de Vaucouleurs, G. 1983a, A6btophy,6. J. Suppt. 51, 549. , and de Vaucouleurs, G. 6. J. 266, l. Charlier, C. 1. 1908, Mil. MILth. A6bton. 6. 4, No. 24. 1. 1922, Mil. Math. A6bton. Phy,6. 16, No. , No. 98. K. 1969, Natune 222, 971. W. 6. J. Lw. • L 113. de Vaucouleurs, G. 1953, A6bton.
Lowe, L. , 1983, "A Catalogue of Galaxies South of Declination -30 0 that have been Observed Spectroscopically", Puhl. of the Department of Astronomy~ Univ. 5. J. , 1983. Mon. Not. R. astr. ~ 203~ 545. , 1983, "Superclusters" to appear in Vol. 21, Ann. Rev. Astr. and Astrophys. 28 A. P. FAIRALL AND H. WINKLER DISCUSSION LORENZ: Can you quote differences in the properties of the Seyfert galaxies as a function of their position in space relative to clusters of galaxies? \LL: As mentioned, there seems to be a tendency for the more distant higher luminosity Seyfert galaxies to prefer open spaces; this is certainly the case for three extreme Seyferts in the sample.
22' I ,, ... *++ J ' , . :+ :. tt: ... '" ••+. ~ • +. " ' " , , ++'. +. , ++ ... ... "' ... +' ... , ...... *. + . ;. + .... :.. /+ + ..... + ++++'" I ' + ... '" • • ,f+ ... + • ... '" '\ ...... . :+ Sc, Sd, Iff, Ow. Sp. V= 3000 10 7500 km r ' .... 1' ... '" + ... + ... ;. +· "' ... + ... '" .. ++.... , , . + "' . . , .. . ",.... : , . +t: • *... . ++ . I .... '" + . '" ~ • ... :. ++: ... ;; ... ,. :+,,+,:. ,. ~ t . : f. " . ,. . " . '. '+, , .. . :'+ : . ' . '. 40' Sb, Sbc V = 3000 10 7500 km r' 5O'~i-~~-~-~-~--~-~-~-~---+ Figure 12.