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.
@doi [ ] 10.1093/mnras/stw206, https://ui.adsabs.harvard.edu/abs/2016MNRAS.457.3101B 457
1 Pith paper cite this work. Polarity classification is still indexing.
1
Pith paper citing it
fields
astro-ph.HE 1years
2026 1verdicts
CONDITIONAL 1representative citing papers
citing papers explorer
-
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.