Astronomy and Astrophysics (ISSN 0004-6361), vol. 244, no. 2, April 1991, p. 351-357.
Mangeney, A.; Daeppen, W.; Praderie, F.; Belmonte, J. A.
Theoretical pulsation frequencies derived from a typical model computation are used to identify the periods during which the Delta Scuti star 63 Herculis oscillates. The frequencies are computed in the adiabatic and linear approximations and consideration is given to p and g modes. The possibility of rotational splitting is considered.