Free Access
Volume 562, February 2014
Article Number A31
Number of page(s) 9
Section Stellar structure and evolution
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

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