Continuous and Burst-like Accretion onto Substellar Companions in Mira Winds

Details Continuous and Burst-like Accretion onto Substellar Companions in Mira Winds Continuous and Burst-like Accretion onto Substellar Companions in Mira Winds

2003-09-12

arxiv.org/abs/astro-ph/0309359v1

Mon.Not.Roy.Astron.Soc.347:173,2004

Astronomy and Astrophysics

Astrophysics

16 pgs., 10 figures with low resolution versions of Figs. 1, 9. Accepted for publication in MNRAS

Scientific paper

10.1111/j.1365-2966.2004.07189.x

We present numerical hydrodynamical modeling of the effects of a giant planet or brown dwarf companion orbiting within the extended atmosphere and wind formation zone of an approximately solar-mass Mira variable star. The large-scale, time-dependent accretion flows within the radially oscillating and outflowing circumstellar gas around Miras are related to Bondi-Hoyle-Lyttleton flows, but have not, to our knowledge, been previously modelled. The new models presented in this paper illustrate the changes in accretion and wake dynamics as the companion mass is varied over a range from 10 to 50 Jupiter masses ($M_J$). The character of the accretion onto the companion changes greatly as the companion mass is increased. At the lowest companion masses considered here, a low continuous rate of mass accretion is punctuated by large, nearly periodic bursts of accretion. When the companion mass is large, the mass accretion has both a continuous part, and a rapidly varying, nearly stochastic part. These trends can be understood as the result of the interplay between the shocks and radial oscillations in the circumstellar gas, and the wake flow behind the companion. Models with accretion bursts may produce observable optical brightenings, and may affect SiO maser emission. (Abridged)

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