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Spectroscopy of LMC Cluster Stars

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arxiv 1910.12922 v1 pith:ZNRJS73K submitted 2019-10-28 astro-ph.SR astro-ph.GA

Andrea K. Dupree , Christian I. Johnson , Mario Mateo , Antonino P. Milone This is my paper · ORCID
classification astro-ph.SRastro-ph.GA
keywords starsclusterh-alphavariableabsorptionaffectallyemission
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High resolution spectra of stars in the ~200 Myr LMC globular cluster, NGC 1866, reveal rapidly rotating stars with variable H-alpha emission and absorption, and signatures of outflowing material. The variable H-alpha line can substanti ally affect photometric measurements obtained with HST/WFC3 narrow-band filters.

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