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Pulsational Mass Ejection in Be Star Disks

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arxiv 1412.8511 v2 pith:7KGCMMFE submitted 2014-12-29 astro-ph.SR

Nathaniel Kee , Stan Owocki , Richard Townsend , Hans-Reinhard Müller This is my paper · ORCID
classification astro-ph.SR
keywords disksejectionmassmaterialmodelmodesnon-radialorbital
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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 contribute to placing material into the circumstellar environment. Several varieties of 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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  1. Using the Coolest Ae Stars to Constrain Circumstellar Disk Viscosity

    astro-ph.SR 2025-06 conditional novelty 6.0 of 10

    Adding viscous shear heating to Ae disk models makes Hα emission much easier to produce for spectral types A2 and cooler, and this dependence is proposed as a new way to measure the disk viscosity parameter α, though ...

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