Magnetic Fields in Massive Stars. I. Dynamo Models

  • Charbonneau P
  • MacGregor K
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Abstract

ABSTRACT Motivated by mounting evidence for the presence of magnetic fields in the atmospheres of" normal" early-type main-sequence stars, we investigate the various possible modes of dynamo action in their convective core. Working within the framework ...

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Charbonneau, P., & MacGregor, K. B. (2001). Magnetic Fields in Massive Stars. I. Dynamo Models. The Astrophysical Journal, 559(2), 1094–1107. https://doi.org/10.1086/322417

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