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Planetary Evaporation and the Dynamics of Planet Wind/Stellar Wind Bow Shocks

We present initial results of a new campaign of simulations focusing on the interaction of planetary winds with stellar environments using Adaptive Mesh Refinement methods. We have confirmed the results of Stone & Proga 2009 that an azimuthal flow structure is created in the planetary wind due to day/night temperatures differences. We show that a backflow towards the planet will occur with a strength that depends on the escape parameter. When a stellar outflow is included, we see unstable bow waves forming through the outflow's interaction with the planetary wind.

preprint2015arXivOpen access
A. FrankB. LiuJ. Carroll-NellenbackA. C. QuillenJ. F. KastingI. Dobbs-DixonE. G. Blackman
astro-ph.EP
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Open access7 authors1 topic
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A. FrankB. LiuJ. Carroll-NellenbackA. C. QuillenJ. F. KastingI. Dobbs-DixonE. G. Blackman

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