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.

Dec 1994

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

Chin. Astron. Astrophys., Vol. 18, No. 4, p. 383 - 392

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Universe: Large-Scale Structure, Infrared Galaxies: Space Distribution

Scientific paper

For four selected fields in the catalogue of IRAS faint sources the authors 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 unnormalized 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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