Nova Scorpii and coalescing low-mass black hole binaries as LIGO sources

Keyphrases

• Black Hole Binaries 100%
• Low-mass 100%
• Novae 100%
• Galaxies 66%
• Supernovae 66%
• Kick 66%
• Mass Transfer 33%
• One-component 33%
• Formation Rate 33%
• Black Hole Mass 33%
• Rate Estimate 33%
• Gravitational Radiation 33%
• Milky Way 33%
• Pulsars 33%
• Black Hole Mergers 33%
• Model Uncertainty 33%
• Initial Mass Function 33%
• Merger Rate 33%
• Chirp Mass 33%
• Neutron Star Binaries 33%
• Black Hole Coalescence 33%
• Spin-up 33%
• Estimated Rates 33%
• Search Volume 33%
• Double Neutron Star 33%

Physics

• Black Holes 100%
• Novae 100%
• Neutron Stars 12%
• Supernovae 12%
• Pulsar 6%
• Gravitational Wave 6%
• Milky Way 6%
• Black Hole Merger 6%
• Initial Mass Function 6%