Staying star gamma Equ
Solar and Stellar Astrophysics
2015-06-23 v1
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.
Cite
@article{arxiv.1506.06235,
title = {Staying star gamma Equ},
author = {V. D. Bychkov and L. V. Bychkova and J. Madej and G. P. Topilskaya},
journal= {arXiv preprint arXiv:1506.06235},
year = {2015}
}
Comments
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