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- Title
General properties of magnetic CP stars.
- Authors
Glagolevskij, Yu.
- Abstract
We present the review of our previous studies related to observational evidence of the fossil field hypothesis of formation and evolution of magnetic and non-magnetic chemically peculiar stars. Analysis of the observed data shows that these stars acquire their main properties in the process of gravitational collapse. In the non-stationary Hayashi phase, a magnetic field becomes weakened and its configuration complicated, but the fossil field global orientation remains. After a non-stationary phase, relaxation of young star's tangled field takes place and by the time of joining ZAMS (Zero Age Main Sequence) it is generally restored to a dipole structure. Stability of dipole structures allows them to remain unchanged up to the end of their life on the Main Sequence which is 10 years at most.
- Subjects
CHEMICALLY peculiar stars; MAGNETIC fields; DATA analysis; GRAVITATIONAL collapse; RELAXATION (Nuclear physics)
- Publication
Astrophysical Bulletin, 2017, Vol 72, Issue 3, p305
- ISSN
1990-3413
- Publication type
Article
- DOI
10.1134/S1990341317030191