The distribution of emission-line galaxies in selected areas of the sky

Details The distribution of emission-line galaxies in selected areas of the sky The distribution of emission-line galaxies in selected areas of the sky

Nov 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988pasp..100.1351m&link_type=abstract

Astronomical Society of the Pacific, Publications (ISSN 0004-6280), vol. 100, Nov. 1988, p. 1351-1353. Research supported by NAS

Astronomy and Astrophysics

Astronomy

2

Emission Spectra, Galactic Clusters, Sky Surveys (Astronomy), Galactic Structure, Mass Distribution, Spatial Distribution, Universe, Voids

Scientific paper

The author discusses the spatial distribution of emission-line galaxies (ELGs) relative to normal galaxies in several areas of the sky. Current evidence supports the notion that ELGs trace a low-density population in all the surveyed areas with the possible exception of the CfA "Slice of the Universe" survey. Based on this and other survey data in the north galactic cap, it is suggested that the ELGs inside the Bootes void may actually define the edge of a totally empty volume within an underdense distribution of normal galaxies.

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