Zobrazeno 1 - 3
of 3
pro vyhledávání: '"Marius Ramsoy"'
Autor:
Taysun Kimm, Adrianne Slyz, Julien Devriendt, Léo Michel-Dansac, Marius Ramsoy, Clotilde Laigle, Martin G. Haehnelt, Jeremy Blaizot, Harley Katz, Joakim Rosdahl, Thibault Garel
Publikováno v:
Monthly Notices of the Royal Astronomical Society
Mon.Not.Roy.Astron.Soc.
Mon.Not.Roy.Astron.Soc., 2020, 494 (2), pp.2200-2220. ⟨10.1093/mnras/staa639⟩
Monthly Notices of the Royal Astronomical Society, 2020, 494 (2), pp.2200-2220. ⟨10.1093/mnras/staa639⟩
Mon.Not.Roy.Astron.Soc.
Mon.Not.Roy.Astron.Soc., 2020, 494 (2), pp.2200-2220. ⟨10.1093/mnras/staa639⟩
Monthly Notices of the Royal Astronomical Society, 2020, 494 (2), pp.2200-2220. ⟨10.1093/mnras/staa639⟩
We use the SPHINX suite of high-resolution cosmological radiation hydrodynamics simulations to study how spatially and temporally inhomogeneous reionization impacts the baryonic content of dwarf galaxies and cosmic filaments. The SPHINX simulations s
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::10c911451e9e8d309908642f8ad55b8c
https://doi.org/10.1093/mnras/staa639
https://doi.org/10.1093/mnras/staa639
Autor:
Taysun Kimm, K. Kraljic, Adrianne Slyz, R. S. Beckmann, Marta Volonteri, Sukyoung K. Yi, Ivan K. Baldry, Sébastien Peirani, R. A. Jackson, Julien Devriendt, Marius Ramsoy, Sugata Kaviraj, Garreth Martin, Yohan Dubois, Hoseung Choi, Christophe Pichon, Thomas M. Sedgwick, Clotilde Laigle
Publikováno v:
Monthly Notices of the Royal Astronomical Society
Monthly Notices of the Royal Astronomical Society, Oxford University Press (OUP): Policy P-Oxford Open Option A, 2021, 502 (3), pp.4262-4276. ⟨10.1093/mnras/stab077⟩
HAL
Monthly Notices of the Royal Astronomical Society, Oxford University Press (OUP): Policy P-Oxford Open Option A, 2021, 502 (3), pp.4262-4276. ⟨10.1093/mnras/stab077⟩
HAL
Low-surface-brightness galaxies (LSBGs) -- defined as systems that are fainter than the surface-brightness limits of past wide-area surveys -- form the overwhelming majority of galaxies in the dwarf regime (M* < 10^9 MSun). Using NewHorizon, a high-r
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::8379b43dd3f4daca4fa6ed08c1ee9dcf
https://hal.archives-ouvertes.fr/hal-03433234
https://hal.archives-ouvertes.fr/hal-03433234
At high redshift, the cosmic web is widely expected to have a significant impact on the morphologies, dynamics and star formation rates of the galaxies embedded within it, underscoring the need for a comprehensive study of the properties of such a fi
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::82d10d3f9e6418b747ed9db98fff568d