2019
DOI: 10.1017/s1743921319006896
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Spectroscopy of LMC cluster stars

Abstract: High resolution spectra of stars in the ≈200 Myr LMC globular cluster, NGC 1866, reveal rapidly rotating stars with variable Hα emission and absorption, and signatures of outflowing material. The variable Hα line can substantially affect photometric measurements obtained with HST/WFC3 narrow-band filters.

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