Molecular hydrogen formation in the interstellar medium: the role of polycyclic aromatic hydrocarbons analysed by the reaction force and activation strain model-Reference-Cited by-同舟云学术

Molecular hydrogen formation in the interstellar medium: the role of polycyclic aromatic hydrocarbons analysed by the reaction force and activation strain model

Published:2018-09-22 Issue:3 Volume:481 Page:3052-3062
ISSN:0035-8711
Container-title:Monthly Notices of the Royal Astronomical Society
language:en
Short-container-title:

Author:

Barrales-Martínez César¹,Cortés-Arriagada Diego²,Gutiérrez-Oliva Soledad¹

Affiliation:

1. Laboratorio de Química Teórica Computacional (QTC), Departamento de Química-Física, Facultad de Química, Pontificia Universidad Católica de Chile, Av. Vicuña Mackenna 4860, 7810000, Macul, Santiago, Chile

2. Programa Institucional de Fomento a la Investigación, Desarrollo e Innovación, Universidad Tecnológica Metropolitana, Ignacio Valdivieso 2409, PO Box 8940577, San Joaquín, Santiago, Chile

Funder

FONDECYT

Publisher

Oxford University Press (OUP)

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

http://academic.oup.com/mnras/article-pdf/481/3/3052/25823217/sty2215.pdf

Reference58 articles.

1. Interstellar polycyclic aromatic hydrocarbons - The infrared emission bands, the excitation/emission mechanism, and the astrophysical implications

2. Hydrogen-graphite interaction: Experimental evidences of an adsorption barrier

3. Understanding reactivity with Kohn-Sham molecular orbital theory: E2-SN2 mechanistic spectrum and other concepts