CARBON ONIONS PRODUCED BY HEAT-TREATMENT OF CARBON SOOT AND THEIR RELATION TO THE 217.5 NM INTERSTELLAR ABSORPTION FEATURE

Citation
Wa. Deheer et D. Ugarte, CARBON ONIONS PRODUCED BY HEAT-TREATMENT OF CARBON SOOT AND THEIR RELATION TO THE 217.5 NM INTERSTELLAR ABSORPTION FEATURE, Chemical physics letters, 207(4-6), 1993, pp. 480-486
Citations number
24
Categorie Soggetti
Physics, Atomic, Molecular & Chemical
Journal title
ISSN journal
00092614
Volume
207
Issue
4-6
Year of publication
1993
Pages
480 - 486
Database
ISI
SICI code
0009-2614(1993)207:4-6<480:COPBHO>2.0.ZU;2-4
Abstract
A new material containing macroscopic quantities of hollow nanometric carbon onions with from 2 to about 8 graphitic shells, with outer diam eters ranging from 3 to 10 nm (characterized by high-resolution electr on microscopy), is produced by heat treatment of pure carbon soot. Oth er structures (i.e. nanotubes) are also formed. Ultraviolet spectra of suspensions of this material in water reveal an absorption band with a peak absorption at 264 nm +/- 3 nm and with widths from 1.4 to 2.0 m um-1. Several features of the absorption spectra closely resemble the interstellar absorption band at 217 nm.