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Paper: Spectroscopic and Photometric Properties of Red Stars in the Bar of the Large Magellanic Cloud
Volume: 310, Variable Stars in the Local Group (IAU Colloquium 193)
Page: 340
Authors: Lloyd Evans, T.
Abstract: Spectroscopy and variability studies of red stars in the Bar of the LMC enable the stars to be classed as spectral type M, S or C and as variables of class L, SR, or Mira. The reults are compared with the data for Magellanic Cloud star clusters and for the galactic field. The number of S stars relative to carbon stars in generally high in comparison to theoretical expectation.
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