Figure 9 from Stellar Evolution in Real Time: Models Consistent with the Direct Observation of a Thermal Pulse in T Ursae Minoris

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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 9.

Predicted (purple) and actual (yellow) sampling locations for each viable pulsation are shown against the seed profile for a model with initial mass 2.5 M_⊙. Blue and green horizontal lines are radial constraints, as in previous figures.

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