WSO/UV: World Space Observatory/Ultraviolet
| dc.creator | Hernanz, M. | |
| dc.creator | Gonzalez-Riestra, R. | |
| dc.creator | Wamsteker, W. | |
| dc.creator | Shustov, B. | |
| dc.creator | Barstow, M. | |
| dc.creator | Brosch, N. | |
| dc.creator | Fu-Zhen, C. | |
| dc.creator | Dennefeld, M. | |
| dc.creator | Dopita, M. | |
| dc.creator | de Castro, A. I. Gomez | |
| dc.creator | Kappelmann, N. | |
| dc.creator | Pagano, I. | |
| dc.creator | Sahade, J. | |
| dc.creator | Haubold, H. | |
| dc.creator | Solheim, J. -E. | |
| dc.creator | Martinez, P. | |
| dc.date | 2002-07-29 | |
| dc.date.accessioned | 2026-07-07T10:31:19Z | |
| dc.date.available | 2026-07-07T10:31:19Z | |
| dc.description | We summarize the capabilities of the World Space Observatory (UV) Project (WSO/UV). An example of the importance of this project (with a planned launch date of 2007/8) for the study of Classical Novae is given. | |
| dc.description | 4 pages, To appear in the proceeedings of the "Classical Nova Explosions" conference, eds. M. Hernanz and J. Jose, AIP | |
| dc.identifier | https://arxiv.org/abs/astro-ph/0207627 | |
| dc.identifier | http://arxiv.org/abs/astro-ph/0207627 | |
| dc.identifier | AIPConf.Proc.637:238-241,2003 | |
| dc.identifier | doi:10.1063/1.1518207 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/178369 | |
| dc.subject | Astrophysics | |
| dc.title | WSO/UV: World Space Observatory/Ultraviolet | |
| dc.type | text |