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Bayesian Inferences on the Twin-star Scenario from NICER Pulsars

  • Authors: Xieyuan Dong, Jinniu Hu, Ying Zhang, Hong Shen

Xieyuan Dong et al 2026 The Astrophysical Journal 1011 .

  • Provider: AAS Journals

Caption: Figure 3.

M–R relations (a) and dimensionless tidal deformability (b) for twin stars derived from the CSS model with specified nuclear matter parameters. The black solid line represents the M–R curve for pure hadronic matter.

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