Dust formation in common envelope binary interactions – II: 3D simulations with self-consistent dust formation

ABSTRACT We performed numerical simulations of the common envelope (CE) interaction between thermally pulsing asymptotic giant branch (AGB) stars of 1.7 and 3.7 M$_{\odot }$, respectively, and a 0.6 M$_{\odot }$ compact companion. We use tabulated equations of state to take into account recombinatio...

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Bibliographic Details
Published in:Monthly notices of the Royal Astronomical Society 2024-09, Vol.533 (1), p.464-481
Main Authors: Bermúdez-Bustamante, Luis C, De Marco, Orsola, Siess, Lionel, Price, Daniel J, González-Bolívar, Miguel, Lau, Mike Y M, Mu, Chunliang, Hirai, Ryosuke, Danilovich, Taïssa, Kasliwal, Mansi M
Format: Article
Language:English
Subjects:
Asymptotic giant branch stars
Binary stars
Carbon stars
Dust
Equations of state
Infrared stars
Nucleation
Simulation
Spectral energy distribution
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