Large-scale two-dimensional distribution of extragalactic IRAS faint sources

Details Large-scale two-dimensional distribution of extragalactic IRAS faint sources Large-scale two-dimensional distribution of extragalactic IRAS faint sources

Oct 1994

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1994cha%26a..18..383b&link_type=abstract

Chinese Astronomy and Astrophysics, Volume 18, Issue 4, p. 383-392.

Astronomy and Astrophysics

Astrophysics

Cosmology-Iras Galaxies-Large-Scale Structure

Scientific paper

For four selected fields in the Catalogue of IRAS Faint Sources we have calculated the two-point correlation function of the galaxies and the correlation fractal dimension. The results show that the galaxies in all the fields are clustered on small angular scales. On larger scales, the distribution can be well expressed by a multi-level fractal. On still larger scales, possible typical scales can be detected using un-normalized pair counts. The average results for the four fields are consistent with previous results for the all-sky IRAS point sources and other sky surveys.

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