Abstract
The evolution of a 1.2M⊙ star along the asymptotic branch with continuous mass loss is presented, showing that this mass loss leads to the formation of a PN with a typical central star in its center.KeywordsMass LossMass Loss RatePlanetary NebulaGiant StarViolent ProcessThese keywords were added by machine and not by the authors. This process is experimental and the keywords may be updated as the learning algorithm improves.
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