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The P(4S) + NH(3Σ) and N(4S) + PH(3Σ) reactions as sources of interstellar phosphorus nitride – CORRIGENDUM

Published online by Cambridge University Press:  13 December 2024

Alexandre C. R. Gomes
Affiliation:
Departamento de Química, Centro Federal de Educação Tecnológica de Minas Gerais, CEFET-MG Av. Amazonas 5253, 30421-169, Belo Horizonte, Minas Gerais, Brazil
André C. Souza
Affiliation:
Departamento de Química, Centro Federal de Educação Tecnológica de Minas Gerais, CEFET-MG Av. Amazonas 5253, 30421-169, Belo Horizonte, Minas Gerais, Brazil
Ahren W. Jasper
Affiliation:
Chemical Sciences and Engineering Division, Argonne National Laboratory, Lemont, IL 60439, USA
Breno R. L. Galvão*
Affiliation:
Departamento de Química, Centro Federal de Educação Tecnológica de Minas Gerais, CEFET-MG Av. Amazonas 5253, 30421-169, Belo Horizonte, Minas Gerais, Brazil
*
Corresponding author: Breno R. L. Galvão; Email: brenogalvao@gmail.com.
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Abstract

Information

Type
Corrigendum
Copyright
© The Author(s), 2024. Published by Cambridge University Press on behalf of Astronomical Society of Australia
Figure 0

Table 1. Rate coefficients as a function of temperature for all reactions studied in this work using a modified Arrhenius equation fit.

Figure 1

Figure 1. Rate coefficients as a function of temperature for the P + NH → N + PH (black) and N + PH → P + NH (blue) reactions. The points refer to the calculated values at fixed temperatures, while the curves are fits to the modified Arrhenius expressions.