Features of the Behavior of Magnetic Chemically Peculiar Stars on the Main Sequence I

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
1. Verfasser: Glagolevskij, Yu. V.
Format: Artikel
Sprache:eng
Schlagworte:
Astronomy
Astrophysics and Cosmology
Deuterium
Magnetic properties
Magnetic stars
Peculiar stars
Physics
Physics and Astronomy
Stellar evolution
Stellar magnetic fields
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Zusammenfassung: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.
ISSN:1990-3413
1990-3421
DOI:10.1134/S1990341321040052