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Paper: Tracing AGB Mass Loss by (Synthetic) High-Resolution IR Spectroscopy
Volume: 378, Why Galaxies Care About AGB Stars: Their Importance as Actors and Probes
Page: 325
Authors: Nowotny, W.; Aringer, B.; Hoefner, S.
Abstract: We report on recent advances in line profile modelling of different near-infrared (NIR) molecular absorption features based on dynamic model atmospheres for pulsating and mass-losing AGB stars (Mira variables).
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