Ennio Poretti and Luciano Mantegazza
Osservatorio Astronomico di Brera, Via E. Bianchi 46, 23807
Merate, Italy
We call attention on the possibility of determining the rotational period of a nonradial pulsating star by combining photometric and spectroscopic techniques. The periods are obtained for three delta Sct stars, i.e. X Cae, BV Cir and HD 2724.