Probable interstellar MgX− (X=CN, NC, CCH, CC, C3N, NCCC, CCNC, C4H, and C4): A DFT study
Author:
Publisher
Elsevier BV
Subject
Space and Planetary Science,Aerospace Engineering,General Earth and Planetary Sciences,Atmospheric Science,Geophysics,Astronomy and Astrophysics
Reference29 articles.
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3. Density-functional thermochemistry. III. The role of exact exchange;Becke;J. Chem. Phys.,1993
4. Photoionization of HCN: the electron affinity and heat of formation of CN;Berkowitz;J. Chem. Phys.,1969
5. Millimeter-wave spectroscopy of vibrationally-excited NaCCH (X2Σ+) and MgCCH (X2Σ+): the ν5 bending mode;Brewster;Chem. Phys. Lett.,1999
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1. New rotational rate coefficients computation of MgC3N(X2Σ+) by collision with He(1S);Monthly Notices of the Royal Astronomical Society;2024-03-01
2. The magnesium paradigm in IRC +10216: Discovery of MgC4H+, MgC3N+, MgC6H+, and MgC5N+;Astronomy & Astrophysics;2023-04
3. Dissociative electron attachment to MgCN;The European Physical Journal D;2020-01
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