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The Dynamical Evolution of the Circumstellar Gas around Low‐ and Intermediate‐Mass Stars. II. The Planetary Nebula Formation
We have studied the effect of the mass of the central star (CS) on the gas evolution during the planetary nebula (PN) phase. We have performed numerical simulations of PN formation using CS tracks for six stellar core masses corresponding to initial masses from 1 to 5 M☉. The gas …