A hybrid SPH/N-body method for star cluster simulations

We present a new hybrid smoothed particle hydrodynamics (SPH)/N-body method for modelling the collisional stellar dynamics of young clusters in a live gas background. By deriving the equations of motion from Lagrangian mechanics we obtain a formally conservative combined SPH-N-body scheme. The SPH g...

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Hauptverfasser: Hubber, David A. (VerfasserIn) , Allison, Richard James (VerfasserIn) , Smith, R. (VerfasserIn) , Goodwin, Simon (VerfasserIn)
Dokumenttyp: Article (Journal)
Sprache:Englisch
Veröffentlicht: 11 April 2013
In: Monthly notices of the Royal Astronomical Society
Year: 2013, Jahrgang: 430, Heft: 3, Pages: 1599-1616
ISSN:1365-2966
DOI:10.1093/mnras/sts694
Online-Zugang:Verlag, lizenzpflichtig, Volltext: https://doi.org/10.1093/mnras/sts694
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Verfasserangaben:D.A. Hubber, R.J. Allison, R. Smith, S.P. Goodwin

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