Show simple item record

dc.creatorKrätschmer, Wolfgangen_US
dc.date.accessioned2006-06-15T15:07:57Z
dc.date.available2006-06-15T15:07:57Z
dc.date.issued1991en_US
dc.identifier1991-WE-2en_US
dc.identifier.urihttp://hdl.handle.net/1811/12567
dc.descriptionAuthor Institution: Max-Planck-Institute f\""{u}r Kernphysiken_US
dc.description.abstractDuring the work in which we attempted to simulate the strong interstellar 217 nm absorption by laboratory produced soot, we noticed UV absorptions which turned out to belong to fullerenes formed along with the soot. This discovery opend the way to produce the fullerene molecules $C_{60}, C_{70}$, and (with a much smaller yield) also larger species in gram quantities. As the most abundant fullerene we obtained the soccerball shaped $C_{60}$ molecule. After extraction from the soot, the fullerenes can be prepared into various ways, e.g. in the form of vapour, amorphous coatings, or crystalline solids, and thus studied in much geater detail than was prevoiusly possible. A status report of our work on the UV and IR spectra of fullerenes will be given.""en_US
dc.format.extent86131 bytes
dc.format.mimetypeimage/jpeg
dc.language.isoEnglishen_US
dc.publisherOhio State Universityen_US
dc.titleFrom Interstellar Dust to Fullerenesen_US
dc.typearticleen_US


Files in this item

Thumbnail

Items in Knowledge Bank are protected by copyright, with all rights reserved, unless otherwise indicated.

This item appears in the following Collection(s)

Show simple item record