A method for defining structures in the distribution of galaxies

Details A method for defining structures in the distribution of galaxies A method for defining structures in the distribution of galaxies

Jan 1994

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1994a%26a...281..964g&link_type=abstract

Astronomy and Astrophysics (ISSN 0004-6361), vol. 281, no. 3, p. 964-966

Astronomy and Astrophysics

Astrophysics

15

Celestial Mechanics, Galactic Clusters, Position (Location), Spatial Distribution, Velocity Distribution, Algorithms, Astronomical Models, Equations Of Motion, Statistical Analysis

Scientific paper

We propose a numerical algorithm for statistical investigation of the
grouping of galaxies, via the construction of a hierarchy of subsystems
in a given system. This algorithm uses the position and velocity
information for the individual galaxies.

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