J/MNRAS/224/453 J/MNRAS/224/453 Velocity data of rich clusters M Colless P Hewett Mon. Not. R. Astron. Soc. 224 453 1987 1987MNRAS.224..453C Clusters, galaxy Redshifts Velocity dispersion We present redshifts and stellar velocity dispersions for about 40 galaxies in each of 14 rich clusters from the southern cluster survey of Abell & Corwin (1983, Early Evolution of the Universe and Its Present Structure, p.179, Eds. Abell & Chincarini, Reidel, Dordrecht, Holland). The clusters cover a wide range of richnesses and Abell and Bautz-Morgan types, our aim being to compile a large, homogeneous database for examining and comparing dynamical phenomena and morphological properties. Further papers will present photometry for the clusters and an analysis of the database.

C02ACO 271700 03.3 -35 57 C03ACO 272100 06.1 -34 43 C19ACO 312603 28.7 -55 43 C20DRCG 0329-5203 30.2 -52 34 C21ACO 45803 45.8 -24 18 AC1Str 0409-59704 09.5 -59 35 C30ACO 333405 18.0 -58 33 C31ACO 336005 40.3 -43 24 C37ACO 370520 41.7 -35 14 C39ACO S 90620 42.3 -51 57 C52ACO 385422 17.7 -35 43 C64ACO 253823 08.7 -19 53 C65ACO 255423 12.3 -21 29 C67Braid 27223 52.1 -34 23

Cluster Cluster name --- Gal Galaxy identifier --- RAh Right ascension (1950) h RAm Right ascension (1950) min RAs Right ascension (1950) s DE- Declination sign --- DEd Declination (1950) deg DEm Declination (1950) arcmin DEs Declination (1950) arcsec cz Heliocentric radial velocity km/s e_cz rms uncertainty on cz km/s sigma Stellar velocity dispersion km/s e_sigma rms uncertainty on sigma km/s R Reliability measure number=1 R: ratio of peak height to noise in the cross-correlation function, which is used to calculate the errors and is a measure of the combined effects of noise and template mismatch (see Tonry & Davis, 1979AJ.....84.1511T). --- Note Notes number=2 Method by which velocities were obtained: Blank: cross-correlation E: emission lines A: absorption features E+A: emission and absorption features --- Marie-Jose Wagner, Patricia Bauer CDS 1997Jun19 UNKNOWN UNKNOWN Prepared via OCR at CDS. * 02-Oct-1997: Four errors detected by H. Andernach were corrected in table3 J_MNRAS_224_453.xml