Hostname: page-component-5c6d5d7d68-ckgrl Total loading time: 0 Render date: 2024-08-19T22:02:28.725Z Has data issue: false hasContentIssue false
  • English
  • Français

Large Scale Clustering in the Universe

Published online by Cambridge University Press:  14 August 2015

P. J. E. Peebles

Extract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

In 1924 Hubble presented the first generally convincing evidence, from the identification of variable stars, that some of the brightest “spiral nebulae” are galaxies of stars well outside the bounds of our own Galaxy. This led him to reconsider the idea that the faint “spiral nebulae,” which were known to be much more abundant than bright ones, might be similar objects at greater distances.

Type
III. Large Scale Systems
Information
Symposium - International Astronomical Union , Volume 79: The Large Scale Structure of the Universe , 1978 , pp. 217 - 226
Copyright
Copyright © Reidel 1978 

References

Abell, G. O.: 1958, Astrophys. J. Suppl. 3, p 211.Google Scholar
de Vaucouleurs, G.: 1971, Publ. Astron. Soc. Pacific 83, p 113.Google Scholar
Dingle, H.: 1933, Monthly Notices Roy. Astron. Soc. 94, p 134.Google Scholar
Einstein, A.: 1917, S. B. Preuss. Akad. Wiss. p 142.Google Scholar
Fath, E. A.: 1914, Astrophys. J. 28, p 84.Google Scholar
Groth, E. J. and Peebles, P. J. E.: 1977, Astrophys. J. 216.Google Scholar
Hauser, M. G. and Peebles, P. J. E.: 1973, Astrophys. J. 185, p 757.Google Scholar
Hubble, E. P.: 1926, Astrophys. J. 64, p 321.Google Scholar
Hubble, E. P.: 1936, Astrophys. J. 84, p 517.Google Scholar
Limber, D. N.: 1954, Astrophys. J. 119, p 655.Google Scholar
Mandelbrot, B. B.: 1975, C. R. 280A, p 1551.Google Scholar
Mandelbrot, B. B.: 1977, Fractals, Freeman, San Francisco.Google Scholar
Milne, E. A.: 1933, Z. Astrophys. 6, p 1.Google Scholar
Neyman, J., Scott, E. L., and Shane, C. D.: 1953, Astrophys. J. 117, p 92.CrossRefGoogle Scholar
Peebles, P. J. E.: 1973, Astrophys. J. 185, p 413.Google Scholar
Peebles, P. J. E. and Hauser, M. G.: 1974, Astrophys. J. Suppl. 28, p 19.Google Scholar
Phillipps, S., Fong, R., Ellis, R. S., Fall, S. M., and Mac Gillivray, H. T.: 1977, preprint.Google Scholar
Rubin, V. C.: 1954, Proc. Nat. Acad. Sci. 40, p 541.Google Scholar
Seldner, M.: 1977, , Princeton University.Google Scholar
Seldner, M. and Peebles, P. J. E.: 1977, Astrophys. J. 215, p 703.CrossRefGoogle Scholar
Shane, C. D.: 1976, private communication.Google Scholar
Shane, C. D. and Wirtanen, C. A.: 1967, Publ. Lick Obs. 22, part 1.Google Scholar
Shapley, H.: 1938, Proc. Nat. Acad. Sci. 24, p 282.Google Scholar
Webster, A.: 1976, Monthly Notices Roy. Astron. Soc. 175, p 71.Google Scholar
Wertz, J. R.: 1971, Astrophys. J. 164, p 227.Google Scholar
Zwicky, F., Herzog, E., Wild, P., Karpowicz, M. and Kowal, C. T.: 1961–1968, Catalogue of Galaxies and Clusters of Galaxies, in 6 vols., California Institute of Technology, Pasadena.Google Scholar