dc.contributor.author |
Dyk, S. Van |
en_US |
dc.contributor.author |
Weiler, K. |
en_US |
dc.contributor.author |
Sramek, R. |
en_US |
dc.contributor.author |
Panagia, N. |
en_US |
dc.contributor.author |
Lacey, C. |
en_US |
dc.contributor.author |
Montes, M. |
en_US |
dc.contributor.author |
Mercaide, J. |
en_US |
dc.contributor.author |
Lewin, W. |
en_US |
dc.contributor.author |
Fox, D. |
en_US |
dc.contributor.author |
Filippenko, A. |
en_US |
dc.contributor.author |
Peng, C. |
en_US |
dc.date.accessioned |
2004-09-23T21:01:06Z |
|
dc.date.available |
2004-09-23T21:01:06Z |
|
dc.date.issued |
2000-08-15 |
en_US |
dc.identifier.citation |
Galaxies and their Contituents at the Highest Angular Resolution |
en_US |
dc.identifier.citation |
Manchester, England |
en_US |
dc.identifier.clearanceno |
00-1431 |
en_US |
dc.identifier.uri |
http://hdl.handle.net/2014/15714 |
|
dc.description.abstract |
The study of supernovae (SNe) and their environments in host galaxies at the highest possible angular resolution in a number of wavelength regimes is providing vital clues to the nature of their progenitor stars. |
en_US |
dc.format.extent |
1701887 bytes |
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dc.format.mimetype |
application/pdf |
|
dc.language.iso |
en_US |
|
dc.subject.other |
supernovae raido astronomy VLBI X-ray Astronomy Galaxies Chandra Hubble Space Telescope |
en_US |
dc.title |
Supernovae at the Highest Angular Resolution |
en_US |