Clusters of Galaxies - Keys to Cosmology
| dc.creator | Schindler, Sabine | |
| dc.date | 2001-09-04 | |
| dc.date.accessioned | 2026-07-07T01:59:50Z | |
| dc.date.available | 2026-07-07T01:59:50Z | |
| dc.description | Various cosmological applications of galaxy clusters are presented. Clusters are used to determine the baryon fraction, dark matter distribution and the matter density of the universe. They also contain a wealth of information about structure formation and evolution on different scales: large-scale structure, cluster formation and also galaxy formation via the interaction of cluster galaxies with the intra-cluster medium. In particular, the X-ray satellites CHANDRA and XMM yield exciting new results for galaxy cluster physics and cosmology. | |
| dc.description | Review given at the Vulcano Workshop 2001, Multifrequency Behaviour of High Energy Cosmic Sources, F. Giovannelli (ed.), 10 pages | |
| dc.identifier | https://arxiv.org/abs/astro-ph/0109040 | |
| dc.identifier | http://arxiv.org/abs/astro-ph/0109040 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/3272 | |
| dc.subject | Astrophysics | |
| dc.title | Clusters of Galaxies - Keys to Cosmology | |
| dc.type | text |