Protoplanetary dynamics - I. Dynamical modes of isothermal protoplanets

Astronomy and Astrophysics – Astronomy

Scientific paper

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Planetary Systems: Formation

Scientific paper

This paper is the first in a series of publications which investigate the stability properties of the complete set of isothermal protoplanetary equilibrium solutions. To perform a non-linear stability analysis, we introduce a fluid dynamics numerical model. We inspect the entire solution set and find five basic dynamical modes: oscillation, pulsation, transition, ejection and collapse.

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