Bibcode
                                    
                            Mangeney, A.; Daeppen, W.; Praderie, F.; Belmonte, J. A.
    Referencia bibliográfica
                                    Astronomy and Astrophysics (ISSN 0004-6361), vol. 244, no. 2, April 1991, p. 351-357.
Fecha de publicación:
    
                        4
            
                        1991
            
  Número de citas
                                    21
                            Número de citas referidas
                                    19
                            Descripción
                                    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.