Are fulleranes responsible for the 21 micron feature?
Author:
Affiliation:
1. School of Physics and Astronomy, Sun Yat-sen University, Zhuhai 519082, China
2. Laboratory for Space Research, Faculty of Science, The University of Hong Kong, Hong Kong, China
Publisher
AIP Publishing
Subject
Physical and Theoretical Chemistry
Link
http://cps.scitation.org/doi/pdf/10.1063/1674-0068/cjcp1911203
Reference27 articles.
1. A 21 micron emission feature in four proto-planetary nebulae
2. CARBON-RICH DUST PAST THE ASYMPTOTIC GIANT BRANCH: ALIPHATICS, AROMATICS, AND FULLERENES IN THE MAGELLANIC CLOUDS
3. ON THE RELATION BETWEEN THE MYSTERIOUS 21μm EMISSION FEATURE OF POST-ASYMPTOTIC GIANT BRANCH STARS AND THEIR MASS-LOSS RATES
4. Circumstellar molecular line absorption and emission in the optical spectra of post-AGB stars
5. Aromatic, aliphatic, and the unidentified 21 micron emission features in proto-planetary nebulae
Cited by 3 articles. 订阅此论文施引文献 订阅此论文施引文献，注册后可以免费订阅5篇论文的施引文献，订阅后可以查看论文全部施引文献
1. Gas-phase Molecules in Protoplanetary Nebulae with the 21 μm Emission Feature;The Astronomical Journal;2024-02-05
2. Molecular Gas in 21 and 30 μm Sources: The 2 mm and 1.3 mm Spectra of IRAS 21318+5631 and 22272+5435;The Astrophysical Journal;2020-08-03
3. Hydrogenated fullerenes (fulleranes) in space;Astrophysics and Space Science;2020-04
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