Chirp mass distribution (IMAGE)
Caption
Distribution of the chirp masses of all binary black-hole mergers observed today. The top panel shows the raw data and probability distributions of the chirp masses of each individual event while the bottom panel shows a model inferred from the combined observations. The gap in chirp masses at 10–12 solar masses and the so-far identified features at about 8, 14, 27 and 45 solar masses are indicated. Figure reproduced from Abbott et al. 2021.
Credit
Abbott et al, 2021. https://journals.aps.org/prx/abstract/10.1103/PhysRevX.11.021053
Usage Restrictions
No restrictions.
License
Public Domain