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Paper: PHOENIX Spectra of Red Supergiants—Varying the Surface Abundances and the Microturbulence
Volume: 425, Hot and Cool: Bridging Gaps in Massive Star Evolution
Page: 61
Authors: Lançon, A.; Hauschildt, P. H.
Abstract: Based on PHOENIX models, we briefly discuss effects of surface abundances and microturbulence on the near-IR spectra of red supergiant stars.
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