The topological characterization of chaos is applied to the irregular
pulsations of a model for a star of the W Virginis type, computed with
a state-of-the-art numerical hydrodynamical code. The banded W Vir at
tractor is found to possess an additional twist when compared to the R
ossler band. It is shown that the stellar light-curve contains the sam
e dynamical information about the attractor as the stellar radius or a
s the radial velocity variations. (C) 1996 American Institute of Physi
cs.