Figure 11 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 11.

Period change rate and bolometric magnitude values from the various TP models. Solid lines are the interpolated values for 10 day period increments. Gray shaded areas are observational constraints. Black and gray dashed lines mark the center and the edges of the best-fitting mass range.

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