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Magnetic Stars After the Hayashi Phase. I

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Astrophysics Aims and scope

The problems of the origin and evolution of magnetic stars based on analysis of observational data are discussed. It is assumed that magnetic stars acquire their major properties during the protostellar collapse stage. The properties of magnetic stars after the Hayashi phase are examined in detail.

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Authors and Affiliations

  1. Special Astrophysical Observatory, Russian Academy of Sciences, Saint Petersburg, Russia

    Yu. V. Glagolevskij

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  1. Yu. V. Glagolevskij
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Correspondence to Yu. V. Glagolevskij.

Additional information

Translated from Astrofizika, Vol. 59, No. 2, pp. 191-212 (May 2016).

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Glagolevskij, Y.V. Magnetic Stars After the Hayashi Phase. I. Astrophysics 59, 164–182 (2016). https://doi.org/10.1007/s10511-016-9425-x

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  • DOI: https://doi.org/10.1007/s10511-016-9425-x

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