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Stellar Evolution in Real Time: Models Consistent with the Direct Observation of a Thermal Pulse in T Ursae Minoris

  • Authors: László Molnár, Meridith Joyce, and László L. Kiss

2019 The Astrophysical Journal 879 62.

  • Provider: AAS Journals

Caption: Figure 7.

The impact of restart effects is demonstrated for a model with initial mass 1.4 M. The black curve line represents the seed profile from which timestamp estimates are drawn. The yellow curve represents a model run from the same initial conditions as the seed mode. Blue and green horizontal lines are as in Figure 6.

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