dc.contributor.author | Hanner, M. S. | en_US |
dc.contributor.author | Hayward, T. L. | en_US |
dc.contributor.author | Lynch, D. K. | en_US |
dc.contributor.author | Russell, R. W. | en_US |
dc.date.accessioned | 2004-09-30T23:18:49Z | |
dc.date.available | 2004-09-30T23:18:49Z | |
dc.date.issued | 1996-10-23 | en_US |
dc.identifier.citation | Tucson, AZ | en_US |
dc.identifier.clearanceno | 96-1341 | en_US |
dc.identifier.uri | http://hdl.handle.net/2014/26468 | |
dc.description.abstract | The spectra of Hale-Bopp were acquired in mid-1996 at R > 3.5 AU. Strong silicate emission is present in all the spectra. The shape of the feature is very similar to that seen in comet P/Halley. This is the first time that a strong silicate feature has been detected in a comet beyond 2 AU. | en_US |
dc.format.extent | 40399 bytes | |
dc.format.mimetype | application/pdf | |
dc.language.iso | en_US | |
dc.subject.other | comet silicate Hale-Bopp spectra | en_US |
dc.title | (abstract) Spectra of Comet Hale-Bopp | en_US |