Hydrodynamic simulations find that realistic circumbinary discs fragment more efficiently than circumstellar discs, yielding more planetary-mass objects with final orbits peaking near 100 AU.
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The formation of circumbinary planets through disc fragmentation
Hydrodynamic simulations find that realistic circumbinary discs fragment more efficiently than circumstellar discs, yielding more planetary-mass objects with final orbits peaking near 100 AU.