File:Neutronstar MassRadius Takami2015 J.Phys.Conf.Ser.600-012056 fig1.svg

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English: TOV sequences for each EOS considered. A shaded yellow band shows current observational constraint on the observed maximum mass in neutron stars, i.e., 2.01 ± 0.04M☉ obtained for the pulsar PSR J0348+0432.
Date
Source (2015). "Constraining the Equation of State of Neutron Stars from Binary Mergers". Journal of Physics: Conference Series 600: 012056. DOI:10.1088/1742-6596/600/1/012056. ISSN 1742-6588. Figure 1
Author Kentaro Takami et al.

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