Supernovae at the Highest Angular Resolution

Dyk, S. Van; Weiler,  K.; Sramek,  R.; Panagia,  N.; Lacey,  C.; Montes,  M.; Mercaide,  J.; Lewin,  W.; Fox,  D.; Filippenko,  A.; Peng,  C.

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