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Multiwavelength Campaign Observations of a Young Solar-type Star, EK Draconis. I. Discovery of Prominence Eruptions Associated with Superflares

  • Authors: Kosuke Namekata, Vladimir S. Airapetian, Pascal Petit, Hiroyuki Maehara, Kai Ikuta, Shun Inoue, Yuta Notsu, Rishi R. Paudel, Zaven Arzoumanian, Antoaneta A. Avramova-Boncheva, Keith Gendreau, Sandra V. Jeffers, Stephen Marsden, Julien Morin, Coralie Neiner, Aline A. Vidotto, Kazunari Shibata

Kosuke Namekata et al 2024 The Astrophysical Journal 961 .

  • Provider: AAS Journals

Caption: Figure 17.

The cross-correlation coefficients for different lag times among light curves for the superflare on 2022 April 17 (E3). The time lags of maximum correlation coefficients, ﹩{r}_{\max }﹩, is defined as the most likely value. The 90th percentile gives the lag time uncertainty. The time delay of X-ray against Hα is ﹩{6}_{-2}^{+3}﹩ minutes, the time delay of X-ray against WL is ﹩{7}_{-2}^{+3}﹩ minutes, the time delay of differential X-ray against Hα is −3﹩{}_{-2}^{+1}﹩ minutes, and the time delay of differential X-ray against WL is −3﹩{}_{-4}^{+2}﹩ minutes. See Tristan et al. (2023) for the method.

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