Abstract
Taking into account the possible influence of external factors such as the orbital motion in binary systems and the rotational velocity on the pulsation of δScuti stars, it may be possible to explain some properties of these variables.
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Antonello, E. (1982). An AD HOC Hypothesis on the Pulsation of Delta Scuti Stars. In: Kopal, Z., Rahe, J. (eds) Binary and Multiple Stars as Tracers of Stellar Evolution. Astrophysics and Space Science Library, vol 98. Springer, Dordrecht. https://doi.org/10.1007/978-94-009-7861-4_5
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DOI: https://doi.org/10.1007/978-94-009-7861-4_5
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