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Supernovae at the Highest Angular Resolution

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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
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


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