阿hedra可为差别旋转体
天体物理学
2007-05-23 v1
摘要
我们利用阿hedra的干涉测量数据探讨其内部旋转规律。对干涉数据重新解释，以及使用修正重力暗化效应和内部星体结构的2D模型，lead us to the conclusion that the star could not be a rigid, near critical, rotator but a differential rotator with the core rotating times faster than the surface.
引用
@article{arxiv.astro-ph/0509173,
title = {Achernar Can be a Differential Rotator},
author = {Juan Zorec and Armando Domiciano De Souza and Yves Fremat and Farok Vakli},
journal= {arXiv preprint arXiv:astro-ph/0509173},
year = {2007}
}
备注
Societe Francaise d'Astronomie et d'Astrophysique, France (2005)