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Isidro Ramírez-Ballinas et al 2019 ApJ 885 116

Archival XMM-Newton observations of the diffuse X-ray emission from the star-forming region LMC-N 57 in the Large Magellanic Cloud unveils the powerful effect of massive stars in destroying their nurseries.

Enrico M. Di Teodoro et al 2019 ApJL 885 L32

The first evidence has been found of molecular gas in two atomic hydrogen (H i) clouds associated with gas outflowing from the Small Magellanic Cloud, likely due to relatively weak starburst-driven winds.

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