[P-AE18] 系外惑星

[PAE18-P05] Starspot mapping and multiwavelength variability for a young solar-type star

*幾田 佳¹、行方 宏介^2,3,4,5、前原 裕之⁵、Airapetian Vladimir^3,4、Petit Pascal⁶、野津 湧太^7,8、野上 大作²、柴田 一成^2,9、EK Dra collaboration (1.東京大学、2.京都大学、3.アメリカ航空宇宙局、4.アメリカン大学、5.国立天文台、6.トゥールーズ大学、7.コロラド大学ボルダー校、8.アメリカ国立太陽天文台、9.同志社大学)

キーワード：太陽型星、恒星黒点、恒星磁場、恒星大気、恒星フレア、G型星

Recent simultaneous multiwavelength observations by the Transiting Exoplanet Survey Satellite (TESS), Seimei telescope, and Neutron star Interior Composition Explorer (NICER), have provided evidence for stellar prominence eruptions associated with superflares on a young solar-type star EK Draconis (EK Dra) (Namekata et al. 2024a). Such superflares are suggested to have been caused by large spots on the polarity inversion line near the stellar limb from the concurrent result of the Zeeman Doppler Imaging (ZDI) at the Bernard Lyot telescope (Namekata et al. 2024b). Thus, to investigate the relation between spot locations from the optical photometry and occurrence of superflares, we perform starspot mapping for the TESS light curve of EK Dra with the code (Ikuta et al. 2020). We also analyze the rotational variability of the TESS light curve, Hα spectrum by the Seimei/KOOLS-IFU, and X-ray data by the NICER, each of which corresponds to the stellar photosphere, chromosphere, and stellar atmosphere (corona), respectively. As a result, we find that (i) some spots are deduced to be near the limb when superflares occurred, (ii) spot locations are consistent with those obtained from the ZDI except for a polar spot, and (iii) the Hα spectrum produced around spots exhibits clear periodicity with respect to the TESS light curve. However, the X-ray data does not show such strong association probably because of multiple spots on the surface and the extended spatial structure of coronal active regions (Ikuta et al., to be submitted). This study enables us to explore the relation between stellar magnetic fields and the stellar atmosphere toward quantifying the stellar XUV radiation to the planetary atmosphere.