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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CITATION STYLE
APA
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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