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.