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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 11.

Absorption spectra of 12C14N and 13C14N at T = 2700 K assuming the isotopic ratio 12C/13C = 7 (C. Sneden et al. 2014) for two small windows in the A and B bands illustrating the relative contribution of 13C14N. Here, a Gaussian line profile with an HWHM of 0.073 cm−1 was used to mimic the observational conditions of WZ Cas, WX Cyg, and TX Psc (R. P. Hedrosa et al. 2013).

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