IDBARKACH, Tijani; MAHAJAN, Thejus; CHABOT, Marin; BÉROFF, Karine; AGUIRRE, Néstor; DÍAZ-TENDERO, Sergio; LAUNOY, Thibaut; LE PADELLEC, Arnaud; PERROT, Luc; BONNIN, Maëlle; LE, Kim Cuong; GESLIN, Florian; DE SEREVILLE, Nicolas; HAMMACHE, Fairouz; JALLAT, Aurélie; MEYER, Anne; CHARON, Émeline; PINO, Thomas; HAMELIN, Thibault; WAKELAM, Valentine

doi:10.1016/j.molap.2018.06.003

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IDBARKACH, Tijani
Institut de Physique Nucléaire d'Orsay [IPNO]

MAHAJAN, Thejus
Institut des Sciences Moléculaires d'Orsay [ISMO]

CHABOT, Marin
Institut de Physique Nucléaire d'Orsay [IPNO]

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Article de revue

Ce document a été publié dans

Molecular Astrophysics. 2018-09, vol. 12, p. 25 - 32

Elsevier

Résumé en anglais

We constructed semiempirical breakdown curves (BDC) for C$_2$N, C$_3$N, C$_2$N$^+$ and C$_3$N$^+$ molecules. These BDC, which are energy dependent dissociation branching ratios (BR) curves, were used to predict products branching ratios for various processes leading to the formation of C$_2$N$^{(+)}$ and C$_3$N$^{(+)}$ excited adducts. These processes, of astrochemical interest, are neutral-neutral and ion-molecule reactions, dissociative recombination and charge transfer reactions with He$^+$. Model predictions of BR are compared to the literature data and to reported values in the kinetic database for astrochemistry KIDA. With the new BR values, the C$_n$N abundances in cold cores were simulated.< Réduire

DOI

http://dx.doi.org/10.1016/j.molap.2018.06.003

Project ANR

Physics of the 2 infinities and the origins - ANR-10-LABX-0038

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Importé de hal

Unités de recherche

Laboratoire d'Astrophysique de Bordeaux (LAB) - UMR 5804