Models of Planets and Brown Dwarfs in Mira Winds
classification
🌌 astro-ph
keywords
browndwarfsmiramodelsplanetsaccretionaffectatmosphere
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We present numerical hydrodynamical models of the effects of planets or brown dwarfs orbiting within the extended atmosphere and wind formation zone of Mira variables. We find time-dependent wake dynamics and episodic accretion phenomena which may give rise to observable optical events and affect SiO maser emission.
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