Low temperature rate constants for the N(4S) + CH(X2Πr) reaction. Implications for N2 formation cycles in dense interstellar clouds-Reference-Cited by-同舟云学术

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Low temperature rate constants for the N(4S) + CH(X2Πr) reaction. Implications for N2 formation cycles in dense interstellar clouds

Published:2013 Issue:33 Volume:15 Page:13888
ISSN:1463-9076
Container-title:Physical Chemistry Chemical Physics
language:en
Short-container-title:Phys. Chem. Chem. Phys.

Author:

Daranlot Julien,Hu Xixi,Xie Changjian,Loison Jean-Christophe,Caubet Philippe,Costes Michel,Wakelam Valentine,Xie Daiqian,Guo Hua,Hickson Kevin M.

Publisher

Royal Society of Chemistry (RSC)

Subject

Physical and Theoretical Chemistry,General Physics and Astronomy

Link

http://pubs.rsc.org/en/content/articlepdf/2013/CP/C3CP52535J

Reference45 articles.

1. Interpolated potential energy surface and dynamics for the reactions between N(4S) and H3+(1A1′)

2. A flowing afterglow selected ion flow tube (FA/SIFT) comparison of SIFT injector flanges and H3+ + N revisited

3. A detailed investigation of proposed gas-phase syntheses of ammonia in dense interstellar clouds

4. Estimates of N2 abundances in dense molecular clouds

5. The interstellar N2 abundance towards HD 124314 from far-ultraviolet observations

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