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| Paper: |
Pulsational Mass Ejection in Be Star Disks |
| Volume: |
506, Bright Emissaries: Be Stars as Messengers of Star-Disk Physics |
| Page: |
47 |
| Authors: |
Kee, N. D.; Owocki, S.; Townsend, R.; Müller, H.-R. |
| Abstract: |
This work explores a Pulsationally Driven Orbital Mass Ejection (PDOME) model for the launching of Classical Be star disks. Under this model, a combination of rapid rotation and non-radial pulsation modes, characterized by their propagation direction and the relative phase of their velocity and density perturbations, are considered. As well, the orbital stability of material launched by such a mechanism is investigated. |
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