(abstract) Spectra of Comet Hale-Bopp

Hanner, M. S.; Hayward, T. L.; Lynch, D. K.; Russell, R. W.

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