Models of quiescent stellar microwave emission
Models for gyrosynchrotron emission from thermal electrons in dMe stellar coronae are developed using the formula for electron emissivity given by Robinson and Melrose (1984). The most physically plausible model also closely fits VIA observations. A comparison of this model to the observations is presented.
KeywordsSpectral Shape Rotational Modulation Thermal Electron Stellar Radius Right Hand
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