A. F. Kholtygin, S. Fabrika, S. Hubrig, G. A. Chuntonov, A. S. Medvedev, Yu. V. Milanova, M. Schoeller, G. G. Valyavin, O. A. Tsiopa, S. V. Boronina
Published 2017-01-03Version 1
We review the measurements of magnetic fields of OB stars and compile a catalog of magnetic OB stars. Based on available data we confirm that magnetic field values are distributed according to a log--normal law with a mean log(B)=2.53 and a standard deviation $\sigma=0.54$. We also investigate the formation of the magnetic field of OBA stars before the Main Sequence (MS).
Comments: 4 pages, 2 figures, in Proc. Conf. "Stars: from collapse to collapse", 2016 October 3-7, Nizhnij Arkhyz, Karachai-Cherkessian Republic, Special Astrophysical Observatory, Russia, uses asp2014.sty
Statistics of magnetic field measurements and evolution of magnetic field of OBA stars
New magnetic field measurements of beta Cephei stars and Slowly Pulsating B stars
Recent developments in determining the evolution of magnetic OB stars
![QR code for arXiv:1701.00739 [astro-ph.SR]](http://oss.arxitics.com/images/favicon.svg)