A new sample of young candidate Bridge stars is identified and shown to align with gas structures, with kinematics implying a ~125 Myr crossing time consistent with the last LMC-SMC interaction.
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2 Pith papers cite this work. Polarity classification is still indexing.
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astro-ph.GA 2years
2026 2representative citing papers
A model where maximum cluster mass scales with star formation rate explains the LMC age gap as resulting from low-SFR periods producing only faint clusters that are now hard to detect.
citing papers explorer
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Characterisation of the Clouds' young stellar Bridge using Gaia DR3
A new sample of young candidate Bridge stars is identified and shown to align with gas structures, with kinematics implying a ~125 Myr crossing time consistent with the last LMC-SMC interaction.
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The apparent Large Magellanic Cloud star cluster age gap
A model where maximum cluster mass scales with star formation rate explains the LMC age gap as resulting from low-SFR periods producing only faint clusters that are now hard to detect.