So far, astronomers have only detected gravitational waves in the form of brief bursts from the mergers of black holes and neutron stars. However, non-merging compact objects can in theory produce a nonstop torrent of gravitational waves, albeit weaker than those emitted by mergers. In particular, low-mass X-ray binary systems, in which a dense neutron star sweeps up matter torn from a close companion star, are likely suspects for emitting continuous gravitational waves.
torrent art models 4 companion disk
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