THE INFRARED-EMISSION SPECTRUM OF GAS-PHASE C60 (BUCKMINSTERFULLERENE)

被引：143

作者：

FRUM, CI ^{[1
]}

ENGLEMAN, R ^{[1
]}

HEDDERICH, HG ^{[1
]}

BERNATH, PF ^{[1
]}

LAMB, LD ^{[1
]}

HUFFMAN, DR ^{[1
]}

机构：

[1] UNIV ARIZONA,DEPT PHYS,TUCSON,AZ 85721

来源：

CHEMICAL PHYSICS LETTERS | 1991年 / 176卷 / 06期

基金：

美国国家航空航天局; 美国国家科学基金会;

关键词：

D O I：

10.1016/0009-2614(91)90245-5

中图分类号：

O64 [物理化学（理论化学）、化学物理学];

学科分类号：

070304 ; 081704 ;

摘要：

The gas-phase infrared spectrum of C60 has been observed in emission with the National Solar Observatory Fourier transform spectrometer at Kitt Peak. Bands attributable to the C60 molecule are found at 527.1, 570.3, 1169.1 and 1406.9 cm-1. Additional emission features are tentatively assigned to C70 or combination bands of C60. A new, strong emission is observed at 1010.2 cm-1 belonging to an unknown molecule. None of these features can be associated with any of the strong emission bands observed so far in astronomical sources.

引用

页码：504 / 508

页数：5

共 21 条

[1]

AJIE H, UNPUB J PHYS CHEM

[2] ATOMS IN CARBON CAGES AS A SOURCE OF INTERSTELLAR DIFFUSE LINES [J].