Magnetocavitation Model for the Formation of Ejection from an Accreting Neutron Star
The process of the plasma ejection formation from the accreting neutron star is investigated. Magnetocavitation model of this process is suggested. According to this model, the plasma ejection is produced because of the magnetospheric destruction associated with the processes of the neutron star quake, resonant interaction of magnetosphere with the accreted plasma and actions of the shock waves from the accretion disk of the neutron star. The suggested model imposes some restrictions on the ejection parametres, nevertheless, the estimations of the ejection parametres obtained in this research are in accordance with the observational data.