Unveiling a connection between large-scale structures behind the southern Milky Way

Details Unveiling a connection between large-scale structures behind the southern Milky Way Unveiling a connection between large-scale structures behind the southern Milky Way

May 1997

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1997mnras.287..472d&link_type=abstract

Monthly Notices of the Royal Astronomical Society, Volume 287, Issue 2, pp. 472-480.

Astronomy and Astrophysics

Astronomy

8

Catalogues, Galaxies: Distances And Redshifts, Large-Scale Structure Of Universe

Scientific paper

A redshift survey of galaxies located in the direction of the southern Milky Way has been carried out using the FLAIR multi-objects system on the 1.2-m UK Schmidt Telescope (UKST) at the Anglo-Australian Observatory in Australia. The galaxy sample was extracted from the LEDA and COSMOS data bases, but essentially by scanning by eye four plates of the UKST/SERC Survey in the region between the Centaurus complex and the Pavo-Indus (PI) wall. The galaxies selected have high central surface brightnesses and are distributed evenly over the whole search area. The majority of the galaxies have apparent magnitudes in the range 11.5

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