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The Maximum Mass and Rotational Kinetic Energy of Rapidly Rotating Neutron Stars

  • Authors: Shao-Peng Tang, Yong-Jia Huang, Yi-Zhong Fan

Shao-Peng Tang et al 2026 The Astrophysical Journal 1000 .

  • Provider: AAS Journals

Caption: Figure 6.

Comparison of the bulk properties of neutron stars derived from the GP (blue) and quarkyonic (gray) models. The corresponding 68.3% credible intervals are indicated above the diagonal subplots.

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