Image Details

Choose export citation format:

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 4.

Top panel: the visual data of T UMi. Middle panel: time–frequency distribution, bottom panel: time–period distribution. The main period is the strongest signal; the average, 313 days, pulsation period is marked with a thin gray dotted line. The black and red dashed lines show the (actual or expected) position of the fundamental period and its harmonics. The white dotted line is the position of the new mode.

Other Images in This Article

Show More

Copyright and Terms & Conditions