Collision-induced state-changing rate coefficients for cyanogen backbones NCN 3Σ− and CNN 3Σ− in astrophysical environments-Reference-Cited by-同舟云学术

Collision-induced state-changing rate coefficients for cyanogen backbones NCN ³Σ⁻ and CNN ³Σ⁻ in astrophysical environments

Published:2023 Issue:44 Volume:25 Page:30330-30342
ISSN:1463-9076
Container-title:Physical Chemistry Chemical Physics
language:en
Short-container-title:Phys. Chem. Chem. Phys.

Author:

González-Sánchez Lola¹^ORCID,Yurtsever Ersin²^ORCID,de la Fuente Jorge Alonso³^ORCID,Sanz-Sanz Cristina³^ORCID,Wester Roland⁴^ORCID,Gianturco Francesco A.⁴^ORCID

Affiliation:

1. Departamento de Química Física, University of Salamanca Plaza de los Caídos sn, 37008, Salamanca, Spain

2. Department of Chemistry, Koc University Rumelifeneriyolu, Sariyer TR 34450, Istanbul, Turkey

3. Departamento de Quimica Fisica Aplicada, Modulo 14, Universidad Autonoma de Madrid, 28049 Madrid, Spain

4. Institut für Ionenphysik und Angewandte Physik, Universität Innsbruck Technikerstr., 25 A-6020, Innsbruck, Austria

Abstract

We report quantum calculations involving the dynamics of rotational energy-transfer processes, by collision with He atoms in, of molecular species which share the presence of the CN backbone considered of importance in interstellar environments.

Funder

Ministerio de Ciencia e Innovación

Publisher

Royal Society of Chemistry (RSC)

Subject

Physical and Theoretical Chemistry,General Physics and Astronomy

Link

http://pubs.rsc.org/en/content/articlepdf/2023/CP/D3CP03316C

Reference42 articles.

1. J.Lequeux , E.Falgarone and C.Ryter , The Interstellar Medium , Springer , Berlin , 2005

2. Rotational (de-)excitation of isocyanogen by collision with helium at low energies

3. MOLECULAR HYDROGEN FORMATION CATALYZED BY POLYCYCLIC AROMATIC HYDROCARBONS IN THE INTERSTELLAR MEDIUM

4. HNC and HCN in Comets

5. The detection of HCN on Jupiter