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- W25378061 abstract "Since stellar activity affects atmospheres of close-in habitable exoplanets, knowledge of a star’s activity level is crucial. Different wavelength ranges yield different possibilities on investigating stellar activity phenomena such as flares and CMEs. We present two approaches to this topic using observations from the FUV and Radio domains. The FUV provides density sensitive line ratios, which show enhancements during stellar flaring. The second approach is dedicated to the decameter wavelength domain, where we use the known correlation between radio decameter type II bursts and CMEs on the Sun. We present promising events on the active M-dwarf AD Leo which show a high probability of being of stellar origin concerning the applied criteria for discriminating between stellar and artificial emission. The detected bursts have parameters similar to solar decameter type III bursts. We present and discuss results of both approaches." @default.
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- W25378061 date "2010-01-01" @default.
- W25378061 modified "2023-10-16" @default.
- W25378061 title "Stellar activity at FUV/Radio wavelengths" @default.
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