Comparison of likely candidate models for Abell cluster structures against the observed distribution

Details Comparison of likely candidate models for Abell cluster structures against the observed distribution Comparison of likely candidate models for Abell cluster structures against the observed distribution

Feb 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991apj...367..393b&link_type=abstract

Astrophysical Journal, Part 1 (ISSN 0004-637X), vol. 367, Feb. 1, 1991, p. 393-398. Research supported by the University of Kans

Astronomy and Astrophysics

Astrophysics

3

Astronomical Models, Cosmology, Galactic Clusters, Baryons, Dark Matter, Red Shift, Spatial Distribution

Scientific paper

The amount of structure in the Abell cluster distribution is compared with a variety of 'likely candidate' models, including a minimal isocurvature baryon model, a low-density universe model with baryons and cosmic strings, and a model with hot dark matter and cosmic strings. The hot dark matter and cosmic string model does best at reproducing the characteristics of the observed data sample.

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