Photometric Properties of Low Redshift Galaxy Clusters
| dc.creator | Barkhouse, W. A. | |
| dc.creator | Yee, H. K. C. | |
| dc.creator | Lopez-Cruz, O. | |
| dc.date | 2000-02-17 | |
| dc.date.accessioned | 2026-07-07T01:52:22Z | |
| dc.date.available | 2026-07-07T01:52:22Z | |
| dc.description | We have recently completed a comprehensive photometric survey of 27 Abell clusters with the 8k mosaic camera on the KPNO 0.9m telescope. Preliminary luminosity functions and dwarf-to-giant galaxy ratios have been calculated for five galaxy clusters (A1185, A1656, A2151, A2152, and A2197). A significant increase in the faint end slope between the inner (0.0-0.75 Mpc) and outer (0.75-1.50 Mpc) luminosity function is measured for A2151 (H_o = 50 km/s/Mpc). All five clusters show a significant dip in the luminosity function at M_R = -19.5. | |
| dc.description | 1 page. To appear in "Cosmic Evolution and Galaxy Formation: Structure, Interactions and Feedback", Eds. J.Franco, E.Terlevich, O.Lopez-Cruz, I.Aretxaga, ASP Conf. Series | |
| dc.identifier | https://arxiv.org/abs/astro-ph/0002358 | |
| dc.identifier | http://arxiv.org/abs/astro-ph/0002358 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/600 | |
| dc.subject | Astrophysics | |
| dc.title | Photometric Properties of Low Redshift Galaxy Clusters | |
| dc.type | text |