Correlation functions for galaxy counts

Details Correlation functions for galaxy counts Correlation functions for galaxy counts

Dec 1978

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1978pazh....4..536f&link_type=abstract

(Pis'ma v Astronomicheskii Zhurnal, vol. 4, Dec. 1978, p. 536-539.) Soviet Astronomy Letters, vol. 4, Nov.-Dec. 1978, p. 288, 28

Astronomy and Astrophysics

Astronomy

3

Astrometry, Galaxies, Brightness, Interstellar Matter, Milky Way Galaxy, Spatial Distribution

Scientific paper

At angular distances greater than 0.4 deg of arc the correlation
functions for counts of galaxies brighter than 19-21 mag reflect mainly
the properties of interstellar matter in the Galaxy. The statistical
sample examined shows hardly any sign of systems whose angular diameter
exceeds 1 deg of arc.

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