Filamentary structure in an objectively-derived deep galaxy sample?

Details Filamentary structure in an objectively-derived deep galaxy sample? Filamentary structure in an objectively-derived deep galaxy sample?

Dec 1986

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986japa....7..293m&link_type=abstract

Journal of Astrophysics and Astronomy (ISSN 0250-6335), vol. 7, Dec. 1986, p. 293-298.

Astronomy and Astrophysics

Astrophysics

2

Astronomical Models, Filaments, Galactic Clusters, Galactic Structure, Mass Distribution, Data Sampling, Monte Carlo Method

Scientific paper

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.

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