Hostname: page-component-cd9895bd7-7cvxr Total loading time: 0 Render date: 2024-12-28T20:46:13.200Z Has data issue: false hasContentIssue false
  • English
  • Français

Analysis of the CFA “Great Wall” Using the Minimal Spanning Tree

Published online by Cambridge University Press:  25 May 2016

S.P. Bhavsar  and
D.A. Lauer
S.P. Bhavsar
Affiliation:
University of Kentucky, Lexington, KY 40506-0055, USA
D.A. Lauer
Affiliation:
University of Kentucky, Lexington, KY 40506-0055, USA

Abstract

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.

MST analysis shows the “Great Wall” as a statistically significant linear feature in the galaxy distribution. It is not as long as visual impressions may suggest. Another “Wall” extends radially, perpendicular to the GW. These two walls intersect at the Coma cluster.

Type
Part II: Contributed Papers
Information
Symposium - International Astronomical Union , Volume 168: Examining the Big Bang and the Diffuse Background Radiations , 1996 , pp. 517 - 519
Copyright
Copyright © Kluwer 1996 

References

Barrow, J.D. and Bhavsar, S.P. (1987), QJRAS, 28, pp. 109–128.Google Scholar
Barrow, J.D., Bhavsar, S.P. and Sonoda, D.H. (1985), MNRAS, 216, pp. 17–35.Google Scholar
Bhavsar, S.P. and Ling, E.N. (1988), Ap. J. Lett, 331, pp. L63–L68.Google Scholar
Geller, M.J. and Huchra, J.P. (1989), Science, 246, pp. 897–903.CrossRefGoogle Scholar
Ramella, M., Geller, M.J. and Huchra, J.P. (1992), Ap. J., 384, pp. 396–402.CrossRefGoogle Scholar