The phase-space distribution function of galaxies in clusters and the secondary peak

Details The phase-space distribution function of galaxies in clusters and the secondary peak The phase-space distribution function of galaxies in clusters and the secondary peak

Jun 1982

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982a%26a...110..238t&link_type=abstract

Astronomy and Astrophysics, vol. 110, no. 2, June 1982, p. 238-240.

Astronomy and Astrophysics

Astrophysics

3

Density Distribution, Distribution Functions, Galactic Clusters, Spatial Distribution, Velocity Distribution, Anisotropy, Astronomical Models

Scientific paper

The relationship between the galaxy velocity distribution and the density profile of clusters is examined under the hypothesis of spherical spatial symmetry. It is shown that an anisotropic and oblate velocity distribution is necessary to obtain stationary clusters with a secondary maximum in the density profile. Existing models accounting for the secondary maximum are examined in the light of this result

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