No change detected in ice absorption bands of EC 53 between phases, with ice abundances higher than typical for embedded protostars.
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3 Pith papers cite this work. Polarity classification is still indexing.
3
Pith papers citing it
years
2026 3verdicts
UNVERDICTED 3representative citing papers
Multi-planet systems produce size-dependent dust traps, asymmetric structures, and eccentric orbits that can hide gaps in synthetic ALMA images and limit grain growth.
Simulations demonstrate that gas-dust interactions produce radial offsets between micron and millimeter dust in gas-bearing debris disks, depending on gas mass, optical depth, and small-grain abundance.
citing papers explorer
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EPISODE IV: Ice Inventory in the Envelope of EC 53
No change detected in ice absorption bands of EC 53 between phases, with ice abundances higher than typical for embedded protostars.
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Dust distribution in circumstellar disks harboring multi-planet systems. II. Super-thermal mass planets
Multi-planet systems produce size-dependent dust traps, asymmetric structures, and eccentric orbits that can hide gaps in synthetic ALMA images and limit grain growth.
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The ALMA survey to Resolve exoKuiper belt Substructures (ARKS) XI: Gas-dust interactions and radial offsets between micron and millimetre-sized grains
Simulations demonstrate that gas-dust interactions produce radial offsets between micron and millimeter dust in gas-bearing debris disks, depending on gas mass, optical depth, and small-grain abundance.