Using a magnetic-field-dependent Eddington limit in binary population synthesis makes neutron-star ULXs more visible with milder beaming and improves agreement with observed X-ray luminosity functions.
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Populations of Neutron Star Ultraluminous X-ray Sources: Mind your b's and B's
Using a magnetic-field-dependent Eddington limit in binary population synthesis makes neutron-star ULXs more visible with milder beaming and improves agreement with observed X-ray luminosity functions.