Abstract
According to a popular notion, the dominant pulsation mode in the g Cephei variables is radial. There is, however, at least one exception to this rule. The exception is 12 Lacertae.
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© 1987 D. Reidel Publishing Company, Dordrecht, Holland
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Jerzykiewicz, M. (1987). Two Comments on the β Cephei Variable 12 Lacertae. In: Lamers, H.J.G.L.M., De Loore, C.W.H. (eds) Instabilities in Luminous Early Type Stars. Astrophysics and Space Science Library, vol 136. Springer, Dordrecht. https://doi.org/10.1007/978-94-009-3901-1_16
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DOI: https://doi.org/10.1007/978-94-009-3901-1_16
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