Taxonomical analysis of the Cancer cluster of galaxies

Details Taxonomical analysis of the Cancer cluster of galaxies Taxonomical analysis of the Cancer cluster of galaxies

Sep 1986

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986mnras.222...49p&link_type=abstract

Monthly Notices of the Royal Astronomical Society (ISSN 0035-8711), vol. 222, Sept. 1, 1986, p. 49-53.

Statistics

Computation

5

Computational Astrophysics, Galactic Clusters, Spatial Distribution, Spiral Galaxies, Taxonomy, Luminosity

Scientific paper

The Cnc cluster of galaxies is investigated using the nonhierarchical-descendent taxonomical classification method in position-velocity space (Fages, 1984; Paturel, 1979; Moles et al., 1985). The 78 Cnc-cluster galaxies brighter than m(p) = 15.18 are assigned to 16 groups, of which only seven are considered probable cluster components. The existence of these substructures, including a binary cluster near the center of the field, is found to confirm the finding of Bothum et al. (1983) that the Cnc cluster does not constitute a unique structure.

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