| 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 |
2002-11-5 |
| 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. |
| dc.format.extent |
242179 bytes |
| dc.format.mimetype |
application/pdf |
| dc.identifier.citation |
AIP Conference Proceedings 637:238-241, 2002 10.1063/1.1518207 |
| dc.identifier.uri |
http://hdl.handle.net/10037/2037 |
| dc.identifier.urn |
URN:NBN:no-uit_munin_1789 |
| dc.language.iso |
eng |
| dc.subject |
VDP::Mathematics and natural science: 400::Physics: 430::Astrophysics, astronomy: 438 |
| dc.subject |
Astrophysics |
| dc.title |
WSO/UV: World Space Observatory/Ultraviolet |
| dc.type |
Journal article |
| dc.type |
Tidsskriftartikkel |
