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Gravitational waves from the first detection of a neutron star - black hole merger (GW200105)
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This shows the gravitational wave emission from a neutron star - black hole system consistent with GW200105. The black hole is roughly 4.7 times the mass of the star and neither is spinning. Due to the significant difference in mass, the star barely suffers any disruption until the end and is engulfed by the black hole almost entirely.
Credit: MAYA Collaboration, Deborah Ferguson, Bhavesh Khamesra, Karan Jani, Deirdre Shoemaker, Miguel Gracia-Linares, Pablo Laguna
Credit: MAYA Collaboration, Deborah Ferguson, Bhavesh Khamesra, Karan Jani, Deirdre Shoemaker, Miguel Gracia-Linares, Pablo Laguna
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