For a GW200115-compatible BHNS with a 3.6 solar mass black hole and 1.5 solar mass neutron star, the neutron star may fill its Roche lobe before the ISCO, hinting at a catastrophic mass-transfer channel that could hide electromagnetic counterparts.
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Combining (post-)Newtonian ideas with quasi-equilibrium (QE) sequence analysis for black hole-neutron star (BHNS) gravitational wave events
For a GW200115-compatible BHNS with a 3.6 solar mass black hole and 1.5 solar mass neutron star, the neutron star may fill its Roche lobe before the ISCO, hinting at a catastrophic mass-transfer channel that could hide electromagnetic counterparts.