快速旋转异星致密星的结构特征：与中子星的显著差异
天体物理学
2010-11-19 v1
摘要
比较快速旋转异星致密星的结构参数与中子星的结构参数，指出显著差异。
引用
@article{arxiv.astro-ph/0111604,
title = {Structure of rapidly rotating strange stars: salient differences from neutron stars},
author = {A. V. Thampan},
journal= {arXiv preprint arXiv:astro-ph/0111604},
year = {2010}
}
备注
6 pages, 5 figs. Econf proceedings style. Presentation at "Compact stars in the QCD Phase diagram", August 15-18, 2001, NORDITA, Copenhagen, Denmark