2025MNRAS.538.3130B


Query : 2025MNRAS.538.3130B

2025MNRAS.538.3130B - Mon. Not. R. Astron. Soc., 538, 3130-3143 (2025/April-3)

Investigating C-D out-of-plane vibrational modes in PAHs as a tool to study interstellar deuterium-containing PAHs.

BURAGOHAIN M., ONAKA T., PATHAK A., VATS A. and SAKON I.

Abstract (from CDS):

Previous as well as recent observations by ISO, Spitzer, AKARI, SOFIA, JWST etc. have revealed various characteristics of mid-infrared emission bands between 3 and 20 $\mu$m. Subsequently, several forms of organics including polycylic aromatic hydrocarbons (PAHs)/PAH-like molecules are proposed as carriers for these bands. Deuterated PAH (PAD) is one such substituted PAH, which is proposed as a potential candidate carrier for weak emission bands at 4.4 and 4.65 $\mu \rm m$, detected towards few astronomical targets and are characteristics of aromatic and aliphatic C-D stretching modes in a PAD molecule, respectively. However, the 4.4 $\mu$m band is not widely detected. In order to validate PADs as carriers for mid-infrared emission bands, an additional alternative tool is crucial. If PAHs are deuterated, they should also possess an inherent signature from the C-D out-of-plane (C-D$\rm _{oop}$) vibrations, which are at the longer wavelength side. In this report, features due to C-D$\rm _{oop}$ modes in PAHs bearing a single to multiple deuterium atoms are reported by performing quantum-chemical calculations. This paper reports that some of the C-D$\rm _{oop}$ vibrations appear at the 14-19 $\mu$m range. Also, the strength of C-D$\rm _{oop}$ modes is not proportional to the D/H ratio in PAHs. In addition, a moderate change in the spectra of deuterated PAHs is observed from that of the undeuterated counterparts, as deuteration would alternate the adjacency class of the C-H bonds and the mass distribution of the molecule. We discuss the efficiency and usefulness of these bands to constrain the form of PAHs emitting mid-infrared emission bands.

Abstract Copyright: © 2025 The Author(s). Published by Oxford University Press on behalf of Royal Astronomical Society.

Journal keyword(s): astrochemistry - molecular data - software: simulations - (ISM:) dust, extinction - ISM: lines and bands - ISM: molecules

Simbad objects: 5

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Number of rows : 5
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 M 42 HII 05 35 16.8 -05 23 15           ~ 4411 0
2 NAME Orion Bright Bar reg 05 35 22.30 -05 24 33.0           ~ 1004 0
3 NAME Horsehead Nebula DNe 05 40 59.0 -02 27 30           ~ 555 0
4 RAFGL 2006 Cld 17 47 02.2 -28 33 20           ~ 12 0
5 NGC 6618 OpC 18 20 47 -16 10.3           ~ 1700 0

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