ALT The research team employed simulations to monitor the movement and development of all the stars within the Hyades, leading them to conclude that the Hyades-born black holes are either still within the cluster or in very close proximity to it. This observation aids in our comprehension of how the presence of black holes influences the development of star clusters and, reciprocally, how star clusters contribute to the generation of gravitational wave sources. The study emerged from a tight-knit partnership involving the University of Padova in Italy, ICUBB-IEEC, the University of Cambridge in the United Kingdom, the European Southern Observatory (ESO), and the National Sun Yat-sen University in China. Image of the Hyades cluster by Maurice F. Toet. Research paper: https://doi.org/10.1093/mnras/stad1925