X-Ray Emission of Solar-Type Stars with Superflares
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.
- Publication:
-
Physics of Magnetic Stars
- Pub Date:
- July 2019
- Bibcode:
- 2019ASPC..518..217R