EDP Sciences
Free Access
Issue
A&A
Volume 562, February 2014
Article Number A31
Number of page(s) 9
Section Stellar structure and evolution
DOI https://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

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