Staying star gamma Equ
arXiv:1506.06235
Abstract
We determined rotational period of practically nonrotating Ap star gamma Equ and claim years. This period is about 35000 times larger than the average rotational period among stars of the same spectral class. Paper discusses possible mechanism explaining the origin of this phenomenon.
In "Science - the basis of the present and the foundation for the future". Proceedings of the III Annual International Conference SKFU "University science - region", Stavropol (Russia), 2015, pp. 144-145