GAS-PHASE ABSORPTIONS OF C60+: A NEW COMPARISON WITH ASTRONOMICAL MEASUREMENTS

被引：37

作者：

Walker, G. A. H. ^{[1
]}

Campbell, E. K. ^{[2
]}

Maier, J. P. ^{[2
]}

Bohlender, D. ^{[3
]}

Malo, L. ^{[4
]}

机构：

[1] 1234 Hewlett Pl, Victoria, BC V8S 4P7, Canada

[2] Univ Basel, Dept Chem, CH-4056 Basel, Switzerland

[3] Natl Res Council Canada, Herzberg Astron & Astrophys, 5071 West Saanich Rd, Victoria, BC V9E 2E7, Canada

[4] CFHT Corp, Kamuela, HI 96743 USA

来源：

ASTROPHYSICAL JOURNAL | 2016年 / 831卷 / 02期

关键词：

ISM:; molecules; DIFFUSE INTERSTELLAR BANDS;

D O I：

10.3847/0004-637X/831/2/130

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

Campbell et al. recently revised, by a few tenths of an angstrom, the wavelengths for their low-temperature laboratory measurements of fullerene C-60(+) bands. This accounts for the perturbation caused by the He atom to the C-60(+)-He spectrum. Here, we demonstrate that the revised laboratory wavelengths improve coincidence with the 9632, 9577, 9428, 9365, and 9348 diffuse interstellar bands detected towards the stars HD 46711, HD 169454, and HD 183143.

引用

页数：5

共 13 条

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