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dc.contributor.authorSolheim, Jan Erik
dc.contributor.authorHernanza, M.
dc.contributor.authorGonzález-Riestra, R.
dc.contributor.authorWamsteker, W.
dc.contributor.authorShustov, B.
dc.contributor.authorBarstow, M.
dc.contributor.authorBrosch, N.
dc.contributor.authorFu-Zhen, C.
dc.contributor.authorDennefeld, M.
dc.contributor.authorDopita, M.
dc.contributor.authorGómez de Castro, A.I.
dc.contributor.authorKappelmannc, N.l.
dc.contributor.authorPagano, I.
dc.contributor.authorSahade, J.
dc.contributor.authorHaubold, H.
dc.contributor.authorSolheim, J.-E.
dc.contributor.authorMartínezc, P.
dc.date.accessioned2009-08-14T09:06:23Z
dc.date.available2009-08-14T09:06:23Z
dc.date.issued2002-11-5
dc.description.abstractWe 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.extent242179 bytes
dc.format.mimetypeapplication/pdf
dc.identifier.citationAIP Conference Proceedings 637:238-241, 2002 10.1063/1.1518207en
dc.identifier.nb-fulltextFulltext http://www.ub.uit.no/munin/bitstream/10037/2037/1/article.pdf
dc.identifier.nb-urnURN URN:NBN:no-uit_munin_1789
dc.identifier.urihttp://hdl.handle.net/10037/2037
dc.identifier.urnURN:NBN:no-uit_munin_1789
dc.language.isoengen
dc.subjectVDP::Mathematics and natural science: 400::Physics: 430::Astrophysics, astronomy: 438en
dc.subjectAstrophysicsen
dc.titleWSO/UV: World Space Observatory/Ultravioleten
dc.typeJournal articleen
dc.typeTidsskriftartikkelen


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