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Spectroscopy of LMC cluster stars

  • A. K. Dupree (a1), C. I. Johnson (a1), M. Mateo (a2) and A. P. Milone (a3)

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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Keywords

Spectroscopy of LMC cluster stars

  • A. K. Dupree (a1), C. I. Johnson (a1), M. Mateo (a2) and A. P. Milone (a3)

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