Models of Planets and Brown Dwarfs in Mira Winds

Details Models of Planets and Brown Dwarfs in Mira Winds Models of Planets and Brown Dwarfs in Mira Winds

2002-07-11

arxiv.org/abs/astro-ph/0207256v1

Astrophys.J. 572 (2002) L83

Astronomy and Astrophysics

Astrophysics

4 pages, 3 figures, follow-up to JAAVSO paper

Scientific paper

10.1086/341485

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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