The Cluster M/L and the Value of Omega_m
| dc.creator | Andernach, H. | |
| dc.creator | Plionis, M. | |
| dc.creator | L'opez-Cruz, O. | |
| dc.creator | Tago, E. | |
| dc.creator | Basilakos, S. | |
| dc.date | 2004-07-05 | |
| dc.date.accessioned | 2026-07-07T02:13:44Z | |
| dc.date.available | 2026-07-07T02:13:44Z | |
| dc.description | From an up-to-date compilation of ACO cluster redshifts and velocity dispersions we extract a homogeneous sample of 459 clusters with robust velocity dispersion. Using the virial theorem to estimate cluster masses, and a correlation between Abell galaxy counts and R-band luminosity, we find a median M/L_R of 174 h_50 M_sun/L_sun. However, if we correct the virial masses according to the X-ray vs. virial mass correlation, as derived from our analysis, we obtain M/L_R ~100 h_50 M_sun/L_sun. These two values of M/L imply a mass content of the Universe of Omega_m ~0.26 and 0.15, respectively. | |
| dc.description | 4 pages, no figures, uses asp2004.sty; to appear in "Nearby Large-Scale Structures and the Zone of Avoidance", eds. A.P. Fairall, P. Woudt, ASP Conf. Series, en prensa, San Francisco: Astronomical Society of the Pacific | |
| dc.identifier | https://arxiv.org/abs/astro-ph/0407098 | |
| dc.identifier | http://arxiv.org/abs/astro-ph/0407098 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/7917 | |
| dc.subject | Astrophysics | |
| dc.title | The Cluster M/L and the Value of Omega_m | |
| dc.type | text |