On the large-scale distribution of faint blue galaxies

Details On the large-scale distribution of faint blue galaxies On the large-scale distribution of faint blue galaxies

Apr 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984pazh...10..175k&link_type=abstract

(Pis'ma v Astronomicheskii Zhurnal, vol. 10, Mar. 1984, p. 175-180) Soviet Astronomy Letters (ISSN 0360-0327), vol. 10, Mar.-Apr

Astronomy and Astrophysics

Astronomy

1

Galactic Clusters, Galactic Structure, Red Shift, Autocorrelation, Local Group (Astronomy), Mass Distribution

Scientific paper

Published observations of 92 faint blue galaxies in a 3 x 3-deg area toward the Local Supercluster, obtained with the 6-m telescope of the Special Astrophysical Observatory at Nizhni Arkhyz are analyzed to determine the large-scale two-point line-of-sight correlation function. The results are presented graphically and discussed. Assuming a Hubble constant of 75 km/sec Mpc, positive correlation zones are found at r = 25 Mpc or less, 65-110 Mpc, and near 175 Mpc, with an anticorrelation zone at 25-65 Mpc. The possibility of a 90-Mpc cycle is considered.

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