Thermal generation of the magnetic field in the surface layers of massive stars
classification
🌌 astro-ph.SR
keywords
starsmagneticmassivemechanismatmospheresconsidereddepartureseffect
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A new magnetic field-generation mechanism based on the Nernst effect is considered in hot massive stars. This mechanism can operate in the upper atmospheres of O and B stars where departures from the LTE form a region with the inverse temperature gradient.
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