Structure of rapidly rotating strange stars: salient differences from neutron stars

Details Structure of rapidly rotating strange stars: salient differences from neutron stars Structure of rapidly rotating strange stars: salient differences from neutron stars

2001-11-30

arxiv.org/abs/astro-ph/0111604v1

eConf C010815:48-53,2002

Astronomy and Astrophysics

Astrophysics

6 pages, 5 figs. Econf proceedings style. Presentation at "Compact stars in the QCD Phase diagram", August 15-18, 2001, NORDIT

Scientific paper

Structure parameters of rapidly rotating strange stars are compared with
those for neutron stars. The salient differences are pointed out.

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