DiRAC 2.5 - the pathway to DiRAC Phase 3
Lead Research Organisation:
University of Cambridge
Department Name: Applied Maths and Theoretical Physics
Abstract
Refer to parent proposal from Leicester - Joint reference: T2414701
Planned Impact
Refer to parent proposal from Leicester - Joint reference: T2414701
Organisations
Publications
Sembolini F
(2016)
nIFTy galaxy cluster simulations - II. Radiative models
in Monthly Notices of the Royal Astronomical Society
Sembolini F
(2016)
nIFTy galaxy cluster simulations - I. Dark matter and non-radiative models
in Monthly Notices of the Royal Astronomical Society
Shen S
(2017)
Chemical enrichment of stars due to accretion from the ISM during the Galaxy's assembly
in Monthly Notices of the Royal Astronomical Society
Smith M
(2019)
Cosmological simulations of dwarfs: the need for ISM physics beyond SN feedback alone
in Monthly Notices of the Royal Astronomical Society
Smith Matthew C.
(2019)
Cosmological simulations of dwarfs: the need for ISM physics beyond SN feedback alone
in Monthly Notices of the Royal Astronomical Society
Smith Matthew C.
(2017)
Supernova feedback in numerical simulations of galaxy formation: separating physics from numerics
in ArXiv e-prints
Viel M
(2017)
Diagnosing galactic feedback with line broadening in the low redshift Lyman-a forest
in Monthly Notices of the Royal Astronomical Society: Letters