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Di Folco E

As seen in: Oxford University Press (OUP)
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On the frequencies of circumbinary discs in protostellar systems

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By Eric L. N, Swarthmore College, Di Folco E
| Oxford University Press (OUP)
ABSTRACT We report the analysis of circumbinary (CB) discs formed in a radiation hydrodynamical simulation of star cluster formation. We consider both pure binary stars and pairs within triple and quadruple systems. The protostellar systems are all young (ages < 105 yrs). We find that the systems that host a CB disc have a median separation of ≈11 au, and the median characteristic radius of the discs is ≈64 au.
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