EDP Sciences
Free access
Volume 562, February 2014
Article Number A31
Number of page(s) 9
Section Stellar structure and evolution
DOI http://dx.doi.org/10.1051/0004-6361/201322024
Published online 04 February 2014

Online material

thumbnail Fig. 1

Fitting of the exponents for neutron, hybrid, and pure quark stars. The adopted EOS are indicated in each panel. Only stable models are shown.

Open with DEXTER

Table 1

Neutron/hybrid/quark stars and EOS: exponents for the function Λ(R).

© ESO, 2014