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https://doi.org/10.1093/mnras/199.2.321
Copy DOIPublication Date: Jun 1, 1982 | |
Citations: 2 |
Self-consistent n = 3 polytropic models with a steady α-effect dynamo operating in the inner 20 per cent by radius are constructed. These axisymmetric models are a first step towards developing self-consistent models of upper main sequence stars with a dynamo field generated in the convective core and pervading the radiative envelope.
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