Philip F. Hopkins
12 ta ish
Centre for Theoretical Physics and Astrophysics
FIRE-2 simulations: physics versus numerics in galaxy formation
Philip F. Hopkins, Andrew Wetzel, Dušan Kereš +25
Maqola20185 iqtibosABIGalaxies on FIRE (Feedback In Realistic Environments): stellar feedback explains cosmologically inefficient star formation
Philip F. Hopkins, Dušan Kereš, José Oñorbe +4
MaqolaOchiq kirish20144 iqtibosABIA general class of Lagrangian smoothed particle hydrodynamics methods and implications for fluid mixing problems
MaqolaOchiq kirish20123 iqtibosABIA new class of accurate, mesh-free hydrodynamic simulation methods
MaqolaOchiq kirish20153 iqtibosABIStellar feedback in galaxies and the origin of galaxy-scale winds
Philip F. Hopkins, Eliot Quataert, Norman Murray
MaqolaOchiq kirish20123 iqtibosABINeutral hydrogen in galaxy haloes at the peak of the cosmic star formation history
Claude‐André Faucher‐Giguère, Philip F. Hopkins, Dušan Kereš +3
MaqolaOchiq kirish20152 iqtibosABIThe galactic dust-up: modelling dust evolution in FIRE
Caleb R Choban, Dušan Kereš, Philip F. Hopkins +3
Maqola20222 iqtibosABIWhere are the most ancient stars in the Milky Way?
Kareem El-Badry, Joss Bland‐Hawthorn, Andrew Wetzel +7
Maqola20182 iqtibosABIEVOLUTION OF INTRINSIC SCATTER IN THE SFR–STELLAR MASS CORRELATION AT 0.5 < z < 3
Peter Kurczynski, Eric Gawiser, Viviana Acquaviva +16
MaqolaOchiq kirish20160 iqtibosABI