Sodium hydride NaH(X1Σ+) in collision with helium He(1S) at low temperature: Potential energy surface and rotational rate coefficients-Reference-Cited by-同舟云学术

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Sodium hydride NaH(X1Σ+) in collision with helium He(1S) at low temperature: Potential energy surface and rotational rate coefficients

Published:2019-03 Issue: Volume:519 Page:21-26
ISSN:0301-0104
Container-title:Chemical Physics
language:en
Short-container-title:Chemical Physics

Author:

Bop Cheikh T.,Faye N.A.B.,Hammami K.

Funder

ICTP

OEA

Publisher

Elsevier BV

Subject

Physical and Theoretical Chemistry,General Physics and Astronomy

Reference39 articles.

1. The fractional ionization in dense interstellar clouds;Oppenheimer;Astrophys. J.,1974

2. Some implications for interstellar molecules of a low electron abundance in dense clouds;Mitchell;Astron. J.,1978

3. The depletion of interstellar elements and the interaction between gas and dust in space;Snow;Astrophys. J.,1975

4. On the abundances of interstellar molecules;Watson;Astrophys. J.,1972

5. Ground state dipole moment of nah;Dagdigian;J. Chem. Phys.,1979

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1. BASECOL2023 scientific content;Astronomy & Astrophysics;2023-12-19

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