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Stellar Spots-Heating and Cooling Diamagnetically
Published online by Cambridge University Press: 12 April 2016
Abstract
Diamagnetic effects as heating and cooling mechanisms at stellar surfaces have been ignored in the past. This is due to the misconseption that the effect, when averaged over a velocity distribution, vanishes. We explore here the relevance of the effect to the observed luminosity and color modulations observed in CP stars.
- Type
- II. Magnetic Fields: Observations and Theories
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- Copyright © Astronomical Society of the Pacific 1993