... cycle[*]
The presence of such single-wave second moment variation in the extremely slowly rotating roAp star $\gamma$ Equ (Kochukhov & Ryabchikova 2001a) is thus confirmed to be a signature of a non-axisymmetric non-dipolar pulsation.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
Copyright ESO 2005