Super-Alfven Expansion of a Nova Shell in the Magnetic Field of Its Core

Astronomy and Astrophysics – Astronomy

Scientific paper

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Scientific paper

We study the effect of nova magnetodipole fields on the dynamics and structure of ejected shells by using a numerical model based on the kinetic-hydrodynamic description of plasma dynamics. Our calculations show that characteristic nonuniformities appear in the distribution of field and plasma perturbations during super-Alfven shell expansion in the circumstellar medium.

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