The HeII project: emission lines of the ionized helium in spectra of flare stars and stellar analogues of the solar coronal ejections – programme for observations at the WSO/Spectrum-UV
Emission lines of the ionized helium in spectra of the UV Cet-type flare dwarf stars are considered in detail. Probably, this emission at the late stages of stellar flares is due to stellar analogues of the coronal mass ejections from the Sun. The observational programme for simultaneous space and ground spectral monitoring is proposed to register such events.
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