Magnetic field of chemically peculiar stars in the Orion OB1 Association
I.I. Romanyuk*, E. Semenko, A. Moiseeva, I. Yakunin and D. Kudryavtsev
September 17, 2022
December 14, 2022
The article presents the results of studies of the magnetic field of chemically peculiar stars in the association of young stars Orion OB1. Our results indicate a sharp drop in the proportion of magnetic stars and a simultaneous decrease in their magnetic field with age. The observations were made with the 6-m BTA telescope of the SAO RAS. On the whole, the obtained data testify in favor of the theory of the relic origin of the magnetic field of chemically peculiar stars. However, the formation process itself may have a number of features that have observational manifestations.
How to cite
Metadata are provided both in "article" format (very similar to INSPIRE) as this helps creating
very compact bibliographies which can be beneficial to authors and
readers, and in "proceeding" format
which is more detailed and complete.