The space distribution of emission-line galaxies

Details The space distribution of emission-line galaxies The space distribution of emission-line galaxies

Aug 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985pazh...11..575s&link_type=abstract

(Pis'ma v Astronomicheskii Zhurnal, vol. 11, Aug. 1985, p. 575-582) Soviet Astronomy Letters (ISSN 0360-0327), vol. 11, July-Aug

Astronomy and Astrophysics

Astronomy

2

Cosmology, Emission Spectra, Galactic Clusters, Spatial Distribution, Astronomical Spectroscopy, Red Shift

Scientific paper

The space distribution of emission-line galaxies from the Second Byurakan Survey is investigated in three 4°×4° fields centered at α = 08h00m, δ = +59°00arcmin; α = 09h50m, δ = +55°00arcmin; α = 11h30m, δ = +59°00arcmin. In the first two fields the regions of higher density of galaxies has been found with voids of about 50 Mpc in size between them. The regions of higher galaxy density possibly consist of a few groups or clusters of galaxies. In the third field a continuous distribution of galaxies is observed up to the distance of 300 Mpc.

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