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With arms wide open: A VLT/MUSE view of the mechanisms driving unwinding spiral arms in cluster galaxies.
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Distinguishing ram pressure from gravitational interactions: Applying the size-shape difference method to real galaxies.
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Investigating the clumpy star formation in an interacting dwarf irregular galaxy.
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The MUSE view of ram pressure stripped galaxies in clusters: the GASP sample.
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Bound star clusters observed in a lensed galaxy 460 Myr after the Big Bang.
Nature, 632, 513-516.