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Paper: X-Ray Emission of Solar-Type Stars with Superflares
Volume: 518, Physics of Magnetic Stars
Page: 217
Authors: Ryspaeva, E. B.
Abstract: We analyse X-ray spectra of 6 solar-type stars with superflares. The results show that the coronal temperatures of the objects do not correlate with stellar parameters that can be associated with the origin of superflares. However, X-ray spectral hardness indicates dependence on these parameters. Most probably, superflares on G-type stars do not correlate with their X-ray emission.
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