File:Neutronstar MassRadius Harry2018 Class.QuantumGrav.35-145010 fig1.svg

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English: Parameters characterizing the properties of neutron stars for different equation-of-state models. The solid, colored curves are the results from the two fiducial models SLy (red) and MS1b (blue). The black curves show alternative equation-of- state models. mass-radius relation.
Date
Source (2018). "Observing and measuring the neutron-star equation-of-state in spinning binary neutron star systems". Classical and Quantum Gravity 35 (14): 145010. DOI:10.1088/1361-6382/aac7e3. ISSN 0264-9381. Figure 1
Author Ian Harry and Tanja Hinderer

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