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Magnetic Stars After the Hayashi Phase. II.

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Astrophysics Aims and scope

The properties of magnetic stars derived from observational data are analyzed. The degree of “magnetic” braking of parent protostars, which depends the magnetic field and mass, is studied. The conditions under which magnetic and “normal” nonmagnetic stars are separated, which appear to depend only on the rotational velocity of the protostars, are examined. The reasons for differences in the average magnitudes of the magnetic field in massive and low-mass magnetic stars are analyzed. The magnetic field structures of magnetic stars and their stability over time (rigidity of rotation) are examined.

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Authors and Affiliations

  1. Special Astrophysical Observatory, Russian Academy of Sciences, Moscow, Russia

    Yu. V. Glagolevskij

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

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Translated from Astrofizika, Vol. 59, No. 3, pp. 359-377 (August 2016).

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Glagolevskij, Y.V. Magnetic Stars After the Hayashi Phase. II.. Astrophysics 59, 321–338 (2016). https://doi.org/10.1007/s10511-016-9438-5

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  • DOI: https://doi.org/10.1007/s10511-016-9438-5

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