Spectroscopic study of 6 galaxies (Brough+, 2007)

Details Spectroscopic study of 6 galaxies (Brough+, 2007) Spectroscopic study of 6 galaxies (Brough+, 2007)

Jul 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008ycat..73781507b&link_type=abstract

VizieR On-line Data Catalog: J/MNRAS/378/1507. Originally published in: 2007MNRAS.378.1507B

Physics

Clusters: Galaxy, Spectroscopy, Radial Velocities, Abundances

Scientific paper

The BGG and BCG galaxy samples were selected from the Group Evolution Multi-wavelength Study (GEMS; Osmond & Ponman, 2004MNRAS.350.1511O; Forbes et al., 2006PASA...23...38F) and the BCG sample presented in Brough et al. (2005MNRAS.364.1354B). In both these samples the galaxy is selected as the brightest galaxy closest to the X-ray centroid, that is, closest to the centre of the potential well of these structures.
(5 data files).

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