All Tables

Table 1: The parameters of the underlying "stellar'' models.
Table 2: Summary of results for models with r₀=0.64. $\cal {M}$ is the measure of the mean nonaxisymmetry of the fields, with ${\cal M}=0, 1$ corresponding to purely axisymmetric solutions and solutions with no axisymmetric part, respectively. Asterisks indicate steady solutions.
Table 3: Summary of results for models with r₀=0.20. $\cal {M}$ is the measure of the mean nonaxisymmetry of the fields, with ${\cal M}=0, 1$ corresponding to purely axisymmetric solutions and solutions with no axisymmetric part, respectively. Asterisks indicate steady solutions, and U that a numerical instability was encountered.
Table 4: Summary of results for models with r₀=0.77. $\cal {M}$ is the measure of the mean nonaxisymmetry of the fields, with ${\cal M}=0, 1$ corresponding to purely axisymmetric solutions and solutions with no axisymmetric part, respectively. Asterisks indicate steady solutions.