Southern Milky Way galaxies velocities (Di Nella+ 1997)

Details Southern Milky Way galaxies velocities (Di Nella+ 1997) Southern Milky Way galaxies velocities (Di Nella+ 1997)

Oct 1997

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1997ycat..72870472d&link_type=abstract

VizieR On-line Data Catalog: J/MNRAS/287/472. Originally published in: 1997MNRAS.287..472D

Computer Science

Galaxy Catalogs, Space Velocities, Morphology

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 (http://www-obs.univ-lyon1.fr/base/) and COSMOS (Cat. ) 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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