Using EoS-specific mass-radius-moment of inertia relations, the paper finds mass constraints for three AMXPs that are nearly EoS-independent, with two sources requiring masses well below one solar mass.
T., Riggio A., Papitto A.
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Accretion-induced spin-up: Implications for mass constraints of AMXPs
Using EoS-specific mass-radius-moment of inertia relations, the paper finds mass constraints for three AMXPs that are nearly EoS-independent, with two sources requiring masses well below one solar mass.