Image Details
Observation of Gravitational Waves from the Coalescence of a 2.5–4.5 M ⊙ Compact Object and a Neutron Star
A. G. Abac et al 2024 The Astrophysical Journal Letters 970 .
Caption: Figure 8.
Posterior on the fraction of NSBH systems detected with GWs that may be EM bright, f EM-bright, depending on the threshold remnant mass required to power a counterpart, ﹩f({M}_{\mathrm{rem}}^{b}\gt {M}_{\mathrm{rem},\min }^{b})﹩. The solid and dashed curves represent different values of the minimum remnant mass ﹩{M}_{\mathrm{rem},\min }^{b}﹩. The teal and gray curves show the analysis results with and without GW230529, respectively.
© 2024. The Author(s). Published by the American Astronomical Society.