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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 2.

Middle: distances of successive (local) light maxima. Left and right: the corresponding periodograms from the early (gray highlighted region in the upper left of middle panel) and late (gray highlighted region in the lower right) sections of the light curve. The “early” region covers truncated JD 32,000 to 41,000 and the “late” region, 54,500 to 58,500.

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