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Spectroscopy of LMC cluster stars
Published online by Cambridge University Press: 11 March 2020
Abstract
High resolution spectra of stars in the ≈200 Myr LMC globular cluster, NGC 1866, reveal rapidly rotating stars with variable H α emission and absorption, and signatures of outflowing material. The variable H α line can substantially affect photometric measurements obtained with HST/WFC3 narrow-band filters.
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- © International Astronomical Union 2020