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Paper: Metallicity Effects in Mira Variables: a Model Study
Volume: 310, Variable Stars in the Local Group (IAU Colloquium 193)
Page: 313
Authors: Scholz, M.; Wood, P.R.
Abstract: M-type Mira models with a moderate deviation from solar metalliticy (2x and 0.5x) have been computed and compared to solar-metallicity models. Selected effects of abundance changes on pulsation properties, atmospheric stratifications, spectral features (colors) and surface brightness distributions are discussed.
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