Structure and kinematics of galaxy clusters I. The redshift catalogue
| dc.creator | Stein, P. | |
| dc.date | 1996-01-12 | |
| dc.date.accessioned | 2026-07-07T02:20:46Z | |
| dc.date.available | 2026-07-07T02:20:46Z | |
| dc.description | An extensive redshift survey has been conducted on a sample of 15 nearby (0.01 < z < 0.05) clusters of galaxies. A total number of 860 redshifts were determined by fitting of emission--lines and/or cross-correlation techniques. Of this sample, 735 galaxies are within 0.2--0.8 Mpc ($H_0$ = 50 km/s/Mpc) of the center of clusters. Approximate morphological types are available for most of the galaxies. A comparison of the present redshifts with published data allows an extensive error analysis. The agreement is excellent with the most modern data, showing a zero point error of 5 km/s and an overall consistency of the measurements and their uncertainties. We estimate our redshifts to have mean random errors around 30 km/s. A population analysis of the clusters will be given in a forthcoming paper. | |
| dc.description | Accepted for publication in Astronomy and Astrophysics Supplements. 7 pages, including figures. Catalogues available from the Author upon request | |
| dc.identifier | https://arxiv.org/abs/astro-ph/9601070 | |
| dc.identifier | http://arxiv.org/abs/astro-ph/9601070 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/10318 | |
| dc.subject | Astrophysics | |
| dc.title | Structure and kinematics of galaxy clusters I. The redshift catalogue | |
| dc.type | text |