The Formation of Fullerenes in Planetary Nebulae

被引：15

作者：

Cami, Jan ^{[1
,2
,3
]}

Peeters, Els ^{[1
,2
,3
]}

Bernard-Salas, Jeronimo ^{[4
,5
]}

Doppmann, Greg ^{[6
]}

De Buizer, James ^{[7
]}

机构：

[1] Univ Western Ontario, Dept Phys & Astron, London, ON N6A 3K7, Canada

[2] Univ Western Ontario, Ctr Planetary Sci & Explorat CPSX, London, ON N6A 3K7, Canada

[3] SETI Inst, 189 Bernardo Ave,Suite 100, Mountain View, CA 94043 USA

[4] Open Univ, Dept Phys Sci, Robert Hooke Bldg, Milton Keynes MK7 6AA, Bucks, England

[5] ACRI ST, 260 Route Pin Montard, F-06904 Sophia Antipolis, France

[6] WM Keck Observ, 65-1120 Mamalahoa Highway, Kamuela, HI 96743 USA

[7] NASA, Ames Res Ctr, USRA, Stratospher Observ Infrared Astron, MS N232-12, Moffett Field, CA 94035 USA

来源：

GALAXIES | 2018年 / 6卷 / 04期

基金：

加拿大自然科学与工程研究理事会;

关键词：

planetary nebulae; fullerenes;

D O I：

10.3390/galaxies6040101

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

In the last decade, fullerenes have been detected in a variety of astrophysical environments, with the majority being found in planetary nebulae. Laboratory experiments have provided us with insights into the conditions and pathways that can lead to fullerene formation, but it is not clear precisely what led to the formation of astrophysical fullerenes in planetary nebulae. We review some of the available evidence, and propose a mechanism where fullerene formation in planetary nebulae is the result of a two-step process where carbonaceous dust is first formed under unusual conditions; then, the fullerenes form when this dust is being destroyed.

引用

页数：6

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