The contribution of galaxies to OMEGA_0
| dc.creator | Salucci, Paolo | |
| dc.creator | Persic, Massimo | |
| dc.date | 1994-02-16 | |
| dc.date.accessioned | 2026-07-07T02:19:05Z | |
| dc.date.available | 2026-07-07T02:19:05Z | |
| dc.description | We estimate the contribution of galaxies to the cosmological density Omega_0 including also their extended dark halos. We find Omega_gal< 0.1, so implying that the matter in galaxies cannot by itself close the Universe but marginally could be baryonic. (latex file)two figures available upon request). | |
| dc.description | 4 pages, preprint SISSA, 24/94/A | |
| dc.identifier | https://arxiv.org/abs/astro-ph/9402040 | |
| dc.identifier | http://arxiv.org/abs/astro-ph/9402040 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/9726 | |
| dc.subject | Astrophysics | |
| dc.title | The contribution of galaxies to OMEGA_0 | |
| dc.type | text |