dc.contributor.author | Solheim, Jan Erik | |
dc.contributor.author | Hernanza, M. | |
dc.contributor.author | González-Riestra, R. | |
dc.contributor.author | Wamsteker, W. | |
dc.contributor.author | Shustov, B. | |
dc.contributor.author | Barstow, M. | |
dc.contributor.author | Brosch, N. | |
dc.contributor.author | Fu-Zhen, C. | |
dc.contributor.author | Dennefeld, M. | |
dc.contributor.author | Dopita, M. | |
dc.contributor.author | Gómez de Castro, A.I. | |
dc.contributor.author | Kappelmannc, N.l. | |
dc.contributor.author | Pagano, I. | |
dc.contributor.author | Sahade, J. | |
dc.contributor.author | Haubold, H. | |
dc.contributor.author | Solheim, J.-E. | |
dc.contributor.author | Martínezc, P. | |
dc.date.accessioned | 2009-08-14T09:06:23Z | |
dc.date.available | 2009-08-14T09:06:23Z | |
dc.date.issued | 2002-11-05 | |
dc.description.abstract | 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 Novae is given. | en |
dc.format.extent | 242179 bytes | |
dc.format.mimetype | application/pdf | |
dc.identifier.citation | AIP Conference Proceedings 637:238-241, 2002 10.1063/1.1518207 | en |
dc.identifier.uri | https://hdl.handle.net/10037/2037 | |
dc.identifier.urn | URN:NBN:no-uit_munin_1789 | |
dc.language.iso | eng | en |
dc.rights.accessRights | openAccess | |
dc.subject | VDP::Mathematics and natural science: 400::Physics: 430::Astrophysics, astronomy: 438 | en |
dc.subject | Astrophysics | en |
dc.title | WSO/UV: World Space Observatory/Ultraviolet | en |
dc.type | Journal article | en |
dc.type | Tidsskriftartikkel | en |