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Cambridge University Press (CUP), Proceedings of the International Astronomical Union, S351(14), p. 97-100, 2019

DOI: 10.1017/s1743921319006896

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Spectroscopy of LMC cluster stars

Journal article published in 2019 by A. K. Dupree ORCID, C. I. Johnson ORCID, M. Mateo, A. P. Milone
This paper was not found in any repository, but could be made available legally by the author.
This paper was not found in any repository, but could be made available legally by the author.

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Abstract

AbstractHigh 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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