2016MNRAS.462.1551Y


Query : 2016MNRAS.462.1551Y

2016MNRAS.462.1551Y - Mon. Not. R. Astron. Soc., 462, 1551-1562 (2016/October-3)

On the aliphatic versus aromatic content of the carriers of the 'unidentified' infrared emission features.

YANG X.J., GLASER R., LI A. and ZHONG J.X.

Abstract (from CDS):

Although it is generally accepted that the unidentified infrared emission (UIE) features at 3.3, 6.2, 7.7, 8.6, and 11.3 µm are characteristic of the stretching and bending vibrations of aromatic hydrocarbon materials, the exact nature of their carriers remains unknown: whether they are free-flying, predominantly aromatic gas-phase molecules, or amorphous solids with a mixed aromatic/aliphatic composition are being debated. Recently, the 3.3 and 3.4 µm features which are commonly respectively attributed to aromatic and aliphatic C-H stretches have been used to place an upper limit of ∼2 per cent on the aliphatic fraction of the UIE carriers (i.e. the number of C atoms in aliphatic chains to that in aromatic rings). Here we further explore the aliphatic versus aromatic content of the UIE carriers by examining the ratio of the observed intensity of the 6.2 µm aromatic C-C feature (I6.2) to that of the 6.85 µm aliphatic C-H deformation feature (I6.85). To derive the intrinsic oscillator strengths of the 6.2 µm stretch (A6.2) and the 6.85 µm deformation (A6.85), we employ density functional theory to compute the vibrational spectra of seven methylated polycyclic aromatic hydrocarbon molecules and their cations. By comparing I6.85/I6.2 with A6.85/A6.2, we derive the fraction of C atoms in methyl(ene) aliphatic form to be at most ∼10 per cent, confirming the earlier finding that the UIE emitters are predominantly aromatic. We have also computed the intrinsic strength of the 7.25 µm feature (A7.25), another aliphatic C-H deformation band. We find that A6.85 appreciably exceeds A7.25. This explains why the 6.85 µm feature is more frequently detected in space than the 7.25 µm feature.

Abstract Copyright: © 2016 The Authors Published by Oxford University Press on behalf of the Royal Astronomical Society

Journal keyword(s): dust, extinction - ISM: lines and bands - ISM: molecules - infrared: ISM - infrared: ISM

Simbad objects: 29

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Number of rows : 29
N Identifier Otype ICRS (J2000)
RA
ICRS (J2000)
DEC
Mag U Mag B Mag V Mag R Mag I Sp type #ref
1850 - 2026
#notes
1 IRAS 00350-7436 C* 00 36 59.5591952376 -74 19 50.255251536 16.88 15.81 14.47 14.25 12.92 C3,2e 32 0
2 OGLE SMC-LPV-4910 pA* 00 44 41.1035011488 -73 21 36.123508332   17.06 15.61 15.44 14.515 G:I 30 0
3 LHA 115-N 29 PN 00 48 36.526 -72 58 00.91 17.72 16.60 16.12 16.5 16.44 ~ 50 0
4 LHA 115-N 54 PN 00 56 05.3840663544 -70 19 25.878681444   16.0       ~ 38 0
5 IRAS 01005+7910 pA* 01 04 45.5109702912 +79 26 46.357116648   11.04 10.87 10.85   B1.7Ibeq 75 0
6 [BSS2007] 255 pA* 01 05 46.4557129824 -71 47 05.274363984           B8Iab 11 0
7 NAME Magellanic Clouds GrG 03 00 -71.0           ~ 7988 0
8 IRAS 04296+3429 pA* 04 32 56.9743899192 +34 36 12.459816288   16.13 14.09 13.64 11.64 G0Ia 149 0
9 IRAS 05063-6908 AB? 05 06 03.670 -69 03 58.76           ~ 13 0
10 IRAS 05073-6752 pA* 05 07 13.9164887208 -67 48 46.719455724           ~ 16 0
11 IRAS 05092-7121 LP* 05 08 35.9127962160 -71 17 30.728295348   20.178 18.379   16.493 ~ 15 0
12 IRAS 05110-6616 pA* 05 11 10.6392128544 -66 12 53.624892600 20.528 18.416 16.629 15.70 14.536 F0Ib 21 0
13 IRAS 05185-6806 Y*O 05 18 28.1480883000 -68 04 04.016015256           ~ 14 0
14 OGLE LMC-LPV-39671 LP* 05 18 45.2552888448 -70 05 34.595618568 20.134 19.207 17.481   15.646 ~ 21 0
15 OGLE LMC-LPV-43685 pA* 05 20 43.8870629914 -69 23 41.139112840 17.618 16.515 15.075 13.92 13.887 F5Ib(e) 23 0
16 IRAS Z05259-7052 pA* 05 25 20.7706707096 -70 50 07.476379728 17.562 16.570 15.335   16.252 A2Ib 15 0
17 IRAS 05289-6617 C* 05 29 02.412 -66 15 27.77   22.276 21.353     C 27 0
18 NAME Orion Bright Bar reg 05 35 22.30 -05 24 33.0           ~ 1004 0
19 IRAS F05361-7121 AB? 05 35 25.8455590488 -71 19 56.650882656           ~ 13 0
20 IRAS 05413-6934 LP* 05 40 54.2741121192 -69 33 18.526425156           ~ 12 0
21 NGC 2023 RNe 05 41 37.9 -02 15 52           ~ 657 1
22 HD 37903 Em* 05 41 38.3891026008 -02 15 32.479650720 7.32 7.94 7.83 7.64 7.52 B3IV 385 0
23 SV* HV 12075 PN 05 58 25.9824484048 -69 44 25.806526886   16.276 15.612 15.236   ~ 23 0
24 IRAS 06111-7023 * 06 10 32.0148170760 -70 24 40.784730372           ~ 10 0
25 HD 184738 PN 19 34 45.2337620448 +30 30 58.950651240   10.41 10.44     [WC9] 976 0
26 NGC 7023 OpC 21 01 36.9 +68 09 48           ~ 739 0
27 NGC 7027 PN 21 07 01.571952 +42 14 10.47120   10.358 8.831 10.157   ~ 2541 1
28 V* V448 Lac pA* 22 24 31.4283564864 +43 43 10.978781916 11.22 10.61 9.69     F7I 115 0
29 HD 235858 pA* 22 29 10.3748806056 +54 51 06.344572284   11.40 9.52 8.47 7.34 G5Ia 264 0

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