Filaments in Warm Dark Matter
| dc.creator | Knebe, Alexander | |
| dc.date | 2002-06-20 | |
| dc.date.accessioned | 2026-07-07T02:04:00Z | |
| dc.date.available | 2026-07-07T02:04:00Z | |
| dc.description | Using Warm Dark Matter rather then Cold Dark Matter we are able to solve the over-production of satellite galaxies orbiting in galactic haloes. Moreover, we can show that this model leads to interesting new results in terms of the history and large-scale distribution of low-mass objects as well as the formation of filamentary structures when being compared to the standard CDM scenario. | |
| dc.description | 1 page, 1 figure, rmaa.cls, to appear in 'Galaxy evolution: theory and observations', Eds. V. Avila-Reese, C. Firmani, C. Frenk, & C. Allen, RevMexAA SC (2002) | |
| dc.identifier | https://arxiv.org/abs/astro-ph/0206346 | |
| dc.identifier | http://arxiv.org/abs/astro-ph/0206346 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/4589 | |
| dc.subject | Astrophysics | |
| dc.title | Filaments in Warm Dark Matter | |
| dc.type | text |