Abstract
CI-CASSCF calculations of transitions between the 360 lowest vibrational energy levels in HCN are discussed, together with results of its application to model stellar atmospheres of cool carbon stars.
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© 1985 D. Reidel Publishing Company, Dordrecht, Holland
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Jørgensen, U.G. (1985). HCN in Stellar Atmospheres — a quantum mechanical calculation. In: Jaschek, M., Keenan, P.C. (eds) Cool Stars with Excesses of Heavy Elements. Astrophysics and Space Science Library, vol 114. Springer, Dordrecht. https://doi.org/10.1007/978-94-009-5325-3_39
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DOI: https://doi.org/10.1007/978-94-009-5325-3_39
Publisher Name: Springer, Dordrecht
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