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Maximum mass limit of neutron stars in scalar-tensor gravity

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Consequences of a strong phase transition in the dense matter equation of state for the rotational evolution of neutron stars

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Astronomy & Astrophysics 600 A39 (2017)
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Evolving neutron star+helium star systems to intermediate-mass binary pulsars

W Tang, D Liu and B Wang
Monthly Notices of the Royal Astronomical Society 490 (1) 752 (2019)
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Hyperonic Stars and the Nuclear Symmetry Energy

Constança Providência, Morgane Fortin, Helena Pais and Aziz Rabhi
Frontiers in Astronomy and Space Sciences 6 (2019)
DOI: 10.3389/fspas.2019.00013
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