Strong Post-merger Gravitational Radiation of GW170817-like Events

The post-merger gravitational-wave (GW) radiation of the remnant formed in the binary neutron star (BNS) coalescence has not been directly measured yet. We show in this work that the properties of the BNS involved in GW170817, additionally constrained by PSR J0030+0451, the lower limit on the maximu...

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Veröffentlicht in:	The Astrophysical journal 2020-12, Vol.904 (2), p.119
Hauptverfasser:	Fan, Yi-Zhong, Jiang, Jin-Liang, Tang, Shao-Peng, Jin, Zhi-Ping, Wei, Da-Ming
Format:	Artikel
Sprache:	eng
Schlagworte:	Astrophysics Binary stars Coalescence Coalescing Gravitation Gravitational energy Gravitational waves Neutron stars Neutrons Pulsars Radiation
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