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Paper: On the Mass-Loss History at the Tip of the AGB
Volume: 378, Why Galaxies Care About AGB Stars: Their Importance as Actors and Probes
Page: 343
Authors: Schoenberner, D.; Steffen, M.
Abstract: We demonstrate by means of radiation-hydrodynamics simulations how the spectral energy distribution (SED) of post-AGB objects depends on the mass-loss properties during evolution off the tip of the AGB.
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