A new Monte Carlo method for dust coagulation ensures global conservation of dust properties and improves small-grain resolution in protoplanetary disk simulations.
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2 Pith papers cite this work. Polarity classification is still indexing.
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astro-ph.EP 2years
2026 2representative citing papers
The high-contrast dust asymmetry in HD 34700A is reproduced by a vortex model, with contrast levels excluding eccentric cavity orbit clustering.
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A Monte Carlo method for tracking dust properties during coagulation in protoplanetary disks
A new Monte Carlo method for dust coagulation ensures global conservation of dust properties and improves small-grain resolution in protoplanetary disk simulations.
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The Circumbinary Disc of HD 34700A II. Analysis of a strong dust asymmetry
The high-contrast dust asymmetry in HD 34700A is reproduced by a vortex model, with contrast levels excluding eccentric cavity orbit clustering.