近乎不自转的星 gamma Equ
太阳与恒星天体物理
2015-06-23 v1
摘要
我们确定了几乎不自转的 Ap 星 gamma Equ 的自转周期，并声称 年。该周期约为同类光谱型恒星平均自转周期的 35000 倍。本文讨论了解释该现象起源的可能机制。
引用
@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}
}
备注
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