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- W56193049 abstract "Selected results relevant to coronal structuring in solar-like single stars based on combined radio and X-ray information are presented. Nonthermal radio and thermal soft X-ray emissions from coronal solar-like stars provide direct information on particle acceleration and coronal heating in the magnetically confined outer atmospheres. The structural relationship between the emission sources is mostly inferred from indirect arguments such as rotational modulation or gyroresonance emission. Direct VLBI provides evidence of resolved, extended coronae on solar-like stars." @default.
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- W56193049 date "1996-01-01" @default.
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- W56193049 title "On radio emission and related X-rays in solar-like stellar coronae" @default.
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- W56193049 doi "https://doi.org/10.1017/s0074180900083509" @default.
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