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Analysis of a magnetohydrodynamic stellar wind

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Abstract

Characteristic features of solutions are analysed around the Alfvénic point. There are three types of solutions through the point.

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Authors and Affiliations

  1. Physics Department, Faculty of Education, Iwate University, Morioka, Japan

    Yasumichi Saito

  2. Department of Astronomy, Faculty of Science, Kyoto University, Kyoto, Japan

    Mamoru Saitō

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  1. Yasumichi Saito
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  2. Mamoru Saitō
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Saito, Y., Saitō, M. Analysis of a magnetohydrodynamic stellar wind. Astrophys Space Sci 119, 33–35 (1986). https://doi.org/10.1007/BF00648807

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  • DOI: https://doi.org/10.1007/BF00648807

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