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(abstract) Spectra of Comet Hale-Bopp

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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


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