Probing binary neutron star mergers in dense environments using afterglow counterparts

Keyphrases

• Afterglow 100%
• Binary Neutron Star Mergers 100%
• Dense Environment 100%
• Kick 66%
• High Density 66%
• High Sensitivity 33%
• Cm(III) 33%
• Long Delay 33%
• Star Formation 33%
• Delay Time 33%
• GW170817 33%
• Low Density 33%
• Electromagnetic Counterparts 33%
• Gravitational Wave Events 33%
• Gravitational Wave Detectors 33%
• Third Generation 33%
• Astronomical Data 33%
• Indirect Evidence 33%
• Multi-messenger Observations 33%
• Neutron Star Binaries 33%

Physics

• Afterglow 100%
• Neutron Star Mergers 100%
• Neutron Stars 33%
• Gravitational Wave 33%
• Star Formation 33%
• Gravitational Wave Detectors 33%
• Electromagnetism 33%