Abstract
The application of the Minimal Spanning Three technique to the description of large scale galaxy distribution shows that it can be roughly described as a network of high density 1D filaments and 2D wall-like condensations.
This is a preview of subscription content, log in via an institution to check access.
Access this chapter
Tax calculation will be finalised at checkout
Purchases are for personal use only
References
J. Barrow, S. Bhavsar, D. Sonoda, MNRAS, 216, 17, 1985
R. van de Weygaert, Ph.D. Thesis, University of Leiden, 1991
A. Doroshkevich, D. Tucker, R. Fong, V. Turchaninov, H. Lin, MNRAS, 322, 369, 2001
M. Kendall, P. Moran, Geometrical Probability, (London: Griffin), 1963
Author information
Authors and Affiliations
Rights and permissions
Copyright information
© 2003 Springer-Verlag New York, Inc.
About this paper
Cite this paper
Doroshkevich, A. (2003). Minimal Spanning Tree Technique. In: Statistical Challenges in Astronomy. Springer, New York, NY. https://doi.org/10.1007/0-387-21529-8_35
Download citation
DOI: https://doi.org/10.1007/0-387-21529-8_35
Publisher Name: Springer, New York, NY
Print ISBN: 978-0-387-95546-9
Online ISBN: 978-0-387-21529-7
eBook Packages: Springer Book Archive