Clustering of galaxies by inverse cascade in a turbulent medium

Details Clustering of galaxies by inverse cascade in a turbulent medium Clustering of galaxies by inverse cascade in a turbulent medium

May 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991mnras.250..157k&link_type=abstract

Monthly Notices of the Royal Astronomical Society (ISSN 0035-8711), vol. 250, May 1, 1991, p. 157-160.

Astronomy and Astrophysics

Astronomy

12

Astronomical Models, Cosmology, Galactic Clusters, Nonlinear Systems, Turbulent Flow, Gravitational Effects, Kolmogoroff Theory, Red Shift, Spatial Distribution, Universe

Scientific paper

A definite physical mechanism based in inverse cascading is suggested which quite naturally yields a bottom-up hierarchical structure for galactic clustering. In this mechanism, nonlinear interactions between small fluid elements in an energetically open nonlinear system facilitate the formation of large coherent stable structures. The clustering of galaxies on all scales is interpreted as the result of this self-organization processes occurring in a turbulent medium.

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