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Gyrosynchrotron Emission from Stellar Coronae
Published online by Cambridge University Press: 25 May 2016
Abstract
We analyze quiescent radio spectra of main-sequence cool stars in terms of a simple gyrosynchrotron model. We find that the underlying (assumed) power-law electron distribution is often very hard, with power-law indices (in dN/dE ∝ E−δ) mostly around δ ≍2–3.5.
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- Copyright © Astronomical Society of the Pacific 2000
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