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Alberto Zonca et al 2015 ApJ 810 70

The extinction profiles of the Magellanic Clouds are successfully modeled by absorption by a population of classical dust grains and a collection of free-flying polycyclic aromatic hydrocarbons.

Maxwell Moe and Rosanne Di Stefano 2015 ApJ 810 61

A study of 221 eclipsing binaries in the LMC suggests that 1) younger eclilpsing binaries tend to reside in dustier environments, and 2) younger eclipsing binaries generally have large eccentricities.

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