R. J. Dodd
Articles written in Journal of Astrophysics and Astronomy
Volume 7 Issue 4 December 1986 pp 293-298
The deep galaxy sample of MacGillivray & Dodd (1980), obtained from purely objective means, is investigated using the technique of Kuhn & Uson (1982) for the presence of structure of a filamentary nature. A variety of synthetic fields of galaxies (including both ‘filament’ and ‘non-filament’ models) generated by means of a computer simulation technique have also been studied for comparison purposes. No strong evidence for filamentary structure in the galaxy distribution is found for this deep sample.
Volume 40 | Issue 6
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