© Published under licence by IOP Publishing Ltd.The form of the outflows generated during the interaction of the accretion disc with the tilted stellar magnetosphere in the propeller regime is studied in the ballistic approach. The problem is solved analytically. Different ways of the flux expansion are considered. The results are applied to the description of the narrow absorption details observed in the spectra of young stars in a blue wing of the sodium D Na I resonance lines.
|Title of host publication||Propeller regime of the accretion onto young stars in the ballistic approach|
|Publication status||Published - 2015|
Shulman, S. G., Grinin, V. P., & Potravnov, I. S. (2015). Propeller regime of the accretion onto young stars in the ballistic approach. In Propeller regime of the accretion onto young stars in the ballistic approach (pp. None) https://doi.org/10.1088/1742-6596/661/1/012012