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Coincidence between Rotational Modulations of Coronal and Photospheric Activities on the Saturated Star AB Dor

  • Authors: Fu-Kun Xu, Shenghong Gu

Fu-Kun Xu and Shenghong Gu 2026 The Astronomical Journal 171 .

  • Provider: AAS Journals

Caption: Figure 3.

Phase-folded SXR rates and ﹩{\rm{RV}}^{\prime} ﹩ curves of all observations. In each panel representing an observation, the horizontal red dotted line qualitatively indicates the quiescent level and zero ﹩{\rm{RV}}^{\prime} ﹩, while the open circles represent the points utilized in deriving the ﹩{\rm{RV}}^{\prime} ﹩ curve in Figure 4. The consecutive rotations are colored as blue, orange, and green, in turn. The red dotted lines in the rate panels depict eye-decided references of flux as 0.9 counts s−1. The horizontal bar in the bottom left panel denotes the integral time of 8000 s of spectra in the sliding mode.

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