Search Results - "Maes, Silke"
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MACE: A Machine-learning Approach to Chemistry Emulation
Published in The Astrophysical journal (01-07-2024)“…Abstract The chemistry of an astrophysical environment is closely coupled to its dynamics, the latter often found to be complex. Hence, to properly model these…”
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magritte, a modern software library for 3D radiative transfer – II. Adaptive ray-tracing, mesh construction, and reduction
Published in Monthly notices of the Royal Astronomical Society (01-12-2020)“…ABSTRACT Radiative transfer is a notoriously difficult and computationally demanding problem. Yet, it is an indispensable ingredient in nearly all…”
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3D hydrodynamical survey of the impact of a companion on the morphology and dynamics of AGB outflow
Published 28-07-2022“…With the use of high-resolution ALMA observations, complex structures that resemble those observed in post-AGB stars and planetary nebulae are detected in the…”
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3D simulations of AGB stellar winds -- II. Ray-tracer implementation and impact of radiation on the outflow morphology
Published 19-04-2023“…A&A 674, A122 (2023) Stars with an initial mass below ~ 8 Msun evolve through the asymptotic giant branch (AGB) phase, during which they develop strong stellar…”
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SPH modelling of AGB wind morphology in hierarchical triple systems \& comparison to observation of R Aql
Published 29-08-2024“…A&A 691, A57 (2024) Asymmetric 3D structures are observed in the outflows of evolved low- and intermediate-mass stars, and are believed to be shaped through…”
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Route towards complete 3D hydro-chemical simulations of companion-perturbed AGB outflows
Published 24-06-2022“…Low- and intermediate mass stars experience a significant mass loss during the last phases of their evolution, which obscures them in a vast, dusty envelope…”
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Magritte, a modern software library for 3D radiative transfer: II. Adaptive ray-tracing, mesh construction and reduction
Published 30-11-2020“…Radiative transfer is a notoriously difficult and computationally demanding problem. Yet, it is an indispensable ingredient in nearly all astrophysical and…”
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Atomium: The astounding complexity of the near circumstellar environment of the M-type AGB star R Hydrae. I. Morpho-kinematical interpretation of CO and SiO emission
Published 15-04-2021“…A&A 651, A82 (2021) Evolved low- to intermediate-mass stars are known to shed their gaseous envelope into a large, dusty, molecule-rich circumstellar nebula…”
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