Fake Massive Black Holes in the Milli-Hertz Gravitational-wave Band

In gravitational-wave (GW) astronomy accurate measurement of the source parameters, such as mass, relies on accurate waveform templates. Currently, templates are developed assuming that a source, such as a stellar-mass binary black hole (BBH), is residing in a vacuum. However, astrophysical models p...

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Veröffentlicht in:	The Astrophysical journal 2020-06, Vol.896 (2), p.171
Hauptverfasser:	Chen, Xian, Xuan, Ze-Yuan, Peng, Peng
Format:	Artikel
Sprache:	eng
Schlagworte:	Accretion Accretion disks Active galactic nuclei Astronomical models Astronomy Astrophysical models Astrophysics Binary stars Black holes Chirp signals Data analysis Error analysis Evolution Gravitation Gravitational wave sources Gravitational waves Hydrodynamics Radiation Stellar cores Stellar evolution Time Waveforms
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