Properties of the post in-spiral common envelope ejecta II: dust formation

22 Jul 2020 Iaconi Roberto Maeda Keiichi Nozawa Takaya De Marco Orsola Reichardt Thomas

We study the formation of dust in the expanding gas ejected as a result of a common envelope binary interaction. In our novel approach, we apply the dust formation model of Nozawa et al. to the outputs of the 3D hydrodynamic SPH simulation performed by Iaconi et al., that involves a giant of 0.88~\ms \ and 83~\rs, with a companion of 0.6~\ms \ placed on the surface of the giant in circular orbit... (read more)

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  • SOLAR AND STELLAR ASTROPHYSICS