Black holes occur across a wide range of masses.
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Stellar black holes form when no stable neutron-star configuration can support a collapsing core or compact-object merger remnant.
supported03
Invisible massive companions in X-ray binaries reveal stellar black holes, gravitational waves measure merging black-hole masses, stellar orbits constrain the Milky Way's central black hole, and active galactic nuclei plus stellar/gas dynamics reveal supermassive black holes in other galaxies.