2023ApJ...944...77D


Query : 2023ApJ...944...77D

2023ApJ...944...77D - Astrophys. J., 944, 77 (2023/February-2)

Direct D-atom Incorporation in Radicals: An Overlooked Pathway for Deuterium Fractionation.

DIAS N., GURUSINGHE R.M., BRODERICK B.M., MILLAR T.J. and SUITS A.G.

Abstract (from CDS):

Direct D-H exchange in radicals is investigated in a quasi-uniform flow employing chirped-pulse millimeter-wave spectroscopy. Inspired by the H-atom catalyzed isomerization of C3H2 reported in our previous study, D-atom reactions with the propargyl (C3H3) radical and its photoproducts were investigated. We observed very efficient D-atom enrichment in the photoproducts through an analogous process of D addition/H elimination to C3H2 isomers occurring at 40 K or below. Cyclic C3HD is the only deuterated isomer observed, consistent with the expected addition/elimination yielding the lowest energy product. The other expected addition/elimination product, deuterated propargyl, is not directly detected, although its presence is inferred by the observations in the latter part of the flow. There, in the high-density region of the flow, we observed both isotopomers of singly deuterated propyne attributed to stabilization of the H+C3H2D or D+C3H3 adducts. The implications of these observations for the deuterium fractionation of hydrocarbon radicals in astrochemical environments is discussed with the support of a monodeuterated chemical kinetic model.

Abstract Copyright: © 2023. The Author(s). Published by the American Astronomical Society.

Journal keyword(s): Astrochemistry - Chemical abundances - Isotopic abundances

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 TMC-1 MoC 04 41 45.9 +25 41 27           ~ 1872 0
2 NAME OMC1 Ridge reg 05 35 13.4 -05 23 07           ~ 131 0
3 NAME Orion Molecular Cloud MoC 05 56 -01.8           ~ 1227 1
4 IRAS 16293-2422 cor 16 32 22.56 -24 28 31.8           ~ 1357 1
5 LDN 483 DNe 18 17 35 -04 39.8           ~ 359 0

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