Features of the Behavior of Magnetic Chemically Peculiar Stars on the Main Sequence I
The behavior of magnetic stars near the Zero Age Main Sequence (ZAMS) is considered. The paper shows that the most probable reason for the negative results of the search for magnetic fields in HAeBe stars is turbulence caused by the burning of deuterium. The magnetic field variability and other prop...
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| Veröffentlicht in: | Astrophysical bulletin 2021-10, Vol.76 (4), p.435-449 |
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| container_title | Astrophysical bulletin |
| container_volume | 76 |
| creator | Glagolevskij, Yu. V. |
| description | The behavior of magnetic stars near the Zero Age Main Sequence (ZAMS) is considered. The paper shows that the most probable reason for the negative results of the search for magnetic fields in HAeBe stars is turbulence caused by the burning of deuterium. The magnetic field variability and other properties of stars are studied as they move along the evolutionary path. |
| doi_str_mv | 10.1134/S1990341321040052 |
| format | Article |
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| fulltext | fulltext |
| identifier | ISSN: 1990-3413 |
| ispartof | Astrophysical bulletin, 2021-10, Vol.76 (4), p.435-449 |
| issn | 1990-3413 1990-3421 |
| language | eng |
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| source | SpringerLink Journals - AutoHoldings |
| subjects | Astronomy Astrophysics and Cosmology Deuterium Magnetic properties Magnetic stars Peculiar stars Physics Physics and Astronomy Stellar evolution Stellar magnetic fields |
| title | Features of the Behavior of Magnetic Chemically Peculiar Stars on the Main Sequence I |
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