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Polycyclic Aromatic Hydrocarbons with Armchair Edges: Potential Emitters in Class B Sources
被引:12
|作者:
Ricca, Alessandra
[1
,2
]
Roser, Joseph E.
[1
,2
]
Peeters, Els
[1
,3
]
Boersma, Christiaan
[2
]
机构:
[1] SETI Inst, Carl Sagan Ctr, 189 Bernardo Ave, Mountain View, CA 94043 USA
[2] NASA, Ames Res Ctr, Mail Stop 245-6, Moffett Field, CA 94035 USA
[3] Univ Western Ontario, Dept Phys & Astron, London, ON N6A 3K7, Canada
基金:
加拿大自然科学与工程研究理事会;
关键词:
astrochemistry;
INTERSTELLAR-EMISSION FEATURE;
RESONANT SEXTET BENZENOIDS;
INFRARED-EMISSION;
PAH EMISSION;
PHOTOCHEMICAL EVOLUTION;
SPECTRA;
FEATURES;
ISOMERS;
NEBULAE;
TRACER;
D O I:
10.3847/1538-4357/ab3124
中图分类号:
P1 [天文学];
学科分类号:
0704 ;
摘要:
We have systematically investigated a series of polycyclic aromatic hydrocarbons (PAHs) with armchair edges that maximize the aromaticity, denoted as Clar PAHs, using density functional theory. Their structures fall into three major categories: branched, intermediate, and armchair. Branched PAHs contain up to 60 carbons, they are eroded and the least stable, and their spectra are the most complex. Armchair PAHs are the most stable and their spectra differ from the nominal PAH spectra by lacking a 11.2 mu m band and having their 7.8 and 8.2 mu m bands coalesce as their size increases. Only intermediate and armchair PAHs have 12.7/13.5 m PAH band intensity ratios that are consistent with observations. The fitting results show that Clar PAH spectra are more consistent with class B than class A sources, with only a few small Clar PAHs contributing to the fit of the class A source IRAS 23133+6050 and large Clar PAHs contributing to the fit of the class B source IRAS 17347-3139, and NGC 7027. Overall, our study suggests that large Clar PAHs are potential emitters in class B sources.
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页数:28
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