Redshift surveys of emission-line galaxies

Details Redshift surveys of emission-line galaxies Redshift surveys of emission-line galaxies

Nov 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988pasp..100.1340g&link_type=abstract

Astronomical Society of the Pacific, Publications (ISSN 0004-6280), vol. 100, Nov. 1988, p. 1340-1342.

Astronomy and Astrophysics

Astronomy

Emission Spectra, Galactic Clusters, Red Shift, Sky Surveys (Astronomy), Galactic Radiation, Spatial Distribution, Voids

Scientific paper

The usefulness of employing samples of emission-line galaxies as alternative means of conducting redshift surveys is discussed. Results in the directions of the Bootes and Coma voids show certain differences. In Bootes approximately ten objects have been identified within the void, but the Coma void appears empty at the same luminosities. The Coma void shows little evidence of having a bubble-like structure; it appears more spongelike. There is a large void behind the Coma/A1367 supercluster that is probably related to the Bootes void.

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