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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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