  AB Dor is a young solar-type star with a surface large-scale magnetic field
$10^2$ to $10^3$ times stronger than the that of the Sun. Although strong
magnetic fields are thought to inhibit coronal mass ejections (CMEs), dimming
signatures typically associated with an eruptive CME were recently observed in
AB Dor. The uninterrupted, long-duration dimming signal suggests that a CME
took place at a high latitude, where it remained in view as the star rotates. A
high-latitude CME is also consistent with observations that indicate that AB
Dor hosts polar active regions. To investigate magnetic confinement in AB Dor,
we conduct a parametric modelling study of twenty-one CMEs at latitudes $\sim
60^\circ$, varying the location, mass and magnetic field strength of an
injected flux rope. Twelve models had the flux rope located in an open magnetic
field region, while the remaining nine were in a closed region. Results show
that CMEs in open-field regions are in general more likely to erupt. The four
eruptive CMEs from closed regions had high free magnetic energies $\gtrsim
3\times 10^{35}$ erg, and ten CMEs, predominantly from the closed-field regions
(8/10) were confined. CMEs in closed-field regions exhibited lower kinetic
energies, since part of the CME energy was expended to overcome magnetic
tension and break open the overlying field. In conclusion our work suggests
that eruptive CMEs in AB Dor may occur in high-latitude regions of open
magnetic field, as the magnetic tension in such regions does not significantly
inhibit the eruption.
