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oai:uvadoc.uva.es:10324/647492024-02-02T10:38:12Zcom_10324_1186com_10324_931com_10324_894col_10324_1404

Lavín Puente, María del Carmen Velasco Sanz, Ana María 2024-01-19T12:25:28Z 2024-01-19T12:25:28Z 2022 The Astrophysical Journal, 941:29 (14pp), 2022 December 10 0004-637X https://uvadoc.uva.es/handle/10324/64749 10.3847/1538-4357/ac9e56 29 1 The Astrophysical Journal 941 1538-4357 Producción Científica Theoretical absorption oscillator strengths and wavelengths for rotational transitions of the C2Π(v′ = 0)-X2Π(v″) bands with v″ = 0–6 of nitric oxide are reported. The Molecular Quantum Defect Orbital method has been used in the calculations and the known interaction between the C2Π(v = 0) Rydberg and the B2Π (v = 7) valence states has been dealt with through an appropriate rovibronic energy matrix. We hope that the reported data may be useful in the analysis of the observed ultraviolet nightglow emission from nitric oxide in the upper atmospheres of Earth, Venus, and Mars. application/pdf eng American Astronomical Society info:eu-repo/semantics/openAccess http://creativecommons.org/licenses/by-nc-nd/4.0/ © 2022. The Author(s). Published by the American Astronomical Society. Attribution-NonCommercial-NoDerivatives 4.0 Internacional Molecular spectroscopy (2095); Line intensities (2084); Line positions (2085) Line intensities (2084) Line positions (2085) Transition Energies and Line Oscillator Strengths of the C2Π(0)-X2Π(0–6) Absorption Bands of Nitric Oxide. A Theoretical Study info:eu-repo/semantics/article info:eu-repo/semantics/publishedVersion https://doi.org/10.3847/1538-4357/ac9e56 SI