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Improved Hot Line Lists for Minor CN Isotopologues in the X2Σ+, A2Π, and B2Σ+ Systems Using Diagonal Born–Oppenheimer Corrections

  • Authors: V. A. Terashkevich, S. V. Kozlov, E. A. Pazyuk, A. V. Stolyarov, S. N. Yurchenko, J. Tennyson

V. A. Terashkevich et al 2026 The Astrophysical Journal Supplement Series 287 .

  • Provider: AAS Journals

Caption: Figure 2.

Residuals of the measured 13C14N wavenumbers (C. Sneden et al. 2014) of A2Π(vA = 0 − 22)–X2Σ+(vX = 0−12) transitions (see Table 3) from their theoretical counterparts evaluated: (1) using the original KTPSYT line list (S. V. Kozlov et al. 2024b) and tacitly assuming the mass-invariant properties of the DBOC functions for all states treated (black circles); (2) with the present mass-dependent ab initio DBOC functions determined only for the X and A states (blue circles); and (3) using the mass-dependent semiempirical DBOC functions for all states treated (red circles). The black frame highlights A2Π(vA = 9)–X2Σ+(vX = 3, 4) bands which undergo strong local perturbations caused by the X2Σ+(vX = 13) state.

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