Structure of rapidly rotating strange stars: salient differences from neutron stars
Astrophysics
2010-11-19 v1
Abstract
Structure parameters of rapidly rotating strange stars are compared with those for neutron stars. The salient differences are pointed out.
Cite
@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}
}
Comments
6 pages, 5 figs. Econf proceedings style. Presentation at "Compact stars in the QCD Phase diagram", August 15-18, 2001, NORDITA, Copenhagen, Denmark