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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… Click to show full abstract
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.
Keywords:
magnetic field;
generation magnetic;
massive stars;
thermal generation
Journal Title: Monthly Notices of the Royal Astronomical Society
Year Published: 2017
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Journal Title: Monthly Notices of the Royal Astronomical Society
Year Published: 2017
Link to full text (if available)
Share on Social Media: Sign Up to like & get
recommendations!