Convergence of smoothed particle hydrodynamics simulations of self-gravitating accretion discs: sensitivity to the implementation of radiative cooling

By Rice W. K. M.   Forgan D. H.   Armitage P. J.  

Monthly Notices of the Royal Astronomical Society, Vol. 420, Iss. 2, 2012-02 ,pp. : 1640-1647

Oxford University Press

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Testing subhalo abundance matching in cosmological smoothed particle hydrodynamics simulations

By Simha Vimal   Weinberg David H.   Davé Romeel   Fardal Mark   Katz Neal   Oppenheimer Benjamin D.  

Monthly Notices of the Royal Astronomical Society, Vol. 423, Iss. 4, 2012-07 ,pp. : 3458-3473

Oxford University Press

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Two-and three-dimensional hydrodynamical simulations of mass transfer in semidetached binaries with explicit radiative cooling and self-absorption in their gaseous envelopes

By Nazarenko V.   Glazunova L.   Shakun L.  

Astronomy Reports, Vol. 49, Iss. 4, 2005-04 ,pp. : 284-294

MAIK Nauka/Interperiodica

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Gas cooling in semi-analytic models and smoothed particle hydrodynamics simulations: are results consistent?

By Saro A.   De Lucia G.   Borgani S.   Dolag K.  

Monthly Notices of the Royal Astronomical Society, Vol. 406, Iss. 2, 2010-08 ,pp. : 729-743

Oxford University Press

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START: smoothed particle hydrodynamics with tree-based accelerated radiative transfer

By Hasegawa K.   Umemura M.  

Monthly Notices of the Royal Astronomical Society, Vol. 407, Iss. 4, 2010-10 ,pp. : 2632-2644

Oxford University Press

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