Magnetic Field Structures of the Stars HD 94660, HD 75049, and HD 154708
Based on published data, we have constructed models for the magnetic structures of three stars with a relatively strong magnetic field. They all have a dipolar structure and do not differ in their properties from the bulk of the magnetic stars. However, they, as well as some other objects with a str...
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| Veröffentlicht in: | Astronomy letters 2024-02, Vol.50 (2), p.148-158 |
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| container_title | Astronomy letters |
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| creator | Glagolevskij, Yu. V. |
| description | Based on published data, we have constructed models for the magnetic structures of three stars with a relatively strong magnetic field. They all have a dipolar structure and do not differ in their properties from the bulk of the magnetic stars. However, they, as well as some other objects with a strong magnetic field, do not obey the direct dependence of the rotation period on the stellar magnetic field strength that is expected from the hypothesis about the loss of angular momentum by its transfer to the surrounding protostellar clouds through magnetic field lines. |
| doi_str_mv | 10.1134/S106377372470004X |
| format | Article |
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| ispartof | Astronomy letters, 2024-02, Vol.50 (2), p.148-158 |
| issn | 1063-7737 1562-6873 |
| language | eng |
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| source | Springer Nature - Complete Springer Journals |
| subjects | Angular momentum Astronomy Astrophysics and Astroparticles Field strength Magnetic fields Magnetic properties Magnetic stars Observations and Techniques Physics Physics and Astronomy Protostars Stars Stellar magnetic fields |
| title | Magnetic Field Structures of the Stars HD 94660, HD 75049, and HD 154708 |
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