Redshift studies of large-scale structure. I - The south Coma void region

Details Redshift studies of large-scale structure. I - The south Coma void region Redshift studies of large-scale structure. I - The south Coma void region

Mar 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988aj.....95..651t&link_type=abstract

Astronomical Journal (ISSN 0004-6256), vol. 95, March 1988, p. 651-661.

Astronomy and Astrophysics

Astronomy

16

Emission Spectra, Galactic Structure, Line Spectra, Red Shift, Stellar Luminosity, Correlation, Error Analysis, Line Of Sight, Northern Hemisphere

Scientific paper

This paper is the first of a series of Steward Observatory redshift surveys aimed at relatively faint galaxy samples covering small areas of the sky of known importance for large-scale-structure programs. This sample of 92 galaxies includes the region 12h30m ≤ α ≤ 13h30m, 18° ≤ δ ≤ 26°, complete to mp ≤ 15.7. The authors find no additional galaxies in the Coma void, and that the void is not well described as a "bubble". The surveyed supercluster regions appear to have a normal luminosity function.

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