The Three Hundred project: The Gizmo-Simba run

Autor: Weiguang Cui, Romeel Dave, Alexander Knebe, Elena Rasia, Meghan Gray, Frazer Pearce, Chris Power, Gustavo Yepes, Dhayaa Anbajagane, Daniel Ceverino, Ana Contreras-Santos, Daniel de Andres, Marco De Petris, Stefano Ettori, Roan Haggar, Qingyang Li, Yang Wang, Xiaohu Yang, Stefano Borgani, Klaus Dolag, Ying Zu, Ulrike Kuchner, Rodrigo Cañas, Antonio Ferragamo, Giulia Gianfagna
Přispěvatelé: UAM. Departamento de Física Teórica, Cui, Weiguang, Dave, Romeel, Knebe, Alexander, Rasia, Elena, Gray, Meghan, Pearce, Frazer, Power, Chri, Yepes, Gustavo, Anbajagane, Dhayaa, Ceverino, Daniel, Contreras-Santos, Ana, De??andres, Daniel, De??petris, Marco, Ettori, Stefano, Haggar, Roan, Li, Qingyang, Wang, Yang, Yang, Xiaohu, Borgani, Stefano, Dolag, Klau, Zu, Ying, Kuchner, Ulrike, Ca??as, Rodrigo, Ferragamo, Antonio, Gianfagna, Giulia
Jazyk: angličtina
Rok vydání: 2022
Předmět:
Zdroj: Cui, W, Dave, R, Knebe, A, Rasia, E, Gray, M, Pearce, F, Power, C, Yepes, G, Anbajagane, D, Ceverino, D, Contreras-Santos, A, Andres, D D, Petris, M D, Ettori, S, Haggar, R, Li, Q, Wang, Y, Yang, X, Borgani, S, Dolag, K, Zu, Y, Kuchner, U, Cañas, R, Ferragamo, A & Gianfagna, G 2022, ' The Three Hundred project: The gizmo-simba run ', Monthly Notices of the Royal Astronomical Society, vol. 514, no. 1, pp. 977-996 . https://doi.org/10.1093/mnras/stac1402
DOI: 10.1093/mnras/stac1402
Popis: Artículo escrito por un elevado número de autores, solo se referencian el que aparece en primer lugar, el nombre del grupo de colaboración, si le hubiere, y los autores pertenecientes a la UAM
We introduce gizmo-simba, a new suite of galaxy cluster simulations within The Three Hundred project. The Three Hundred consists of zoom re-simulations of 324 clusters with M 200 ≳ 1014.8, M ⊙ drawn from the MultiDark-Planck N-body simulation, run using several hydrodynamic and semi-analytical codes. The gizmo-simba suite adds a state-of-the-art galaxy formation model based on the highly successful Simba simulation, mildly re-calibrated to match z = 0 cluster stellar properties. Comparing to The Three Hundred zooms run with gadget-x, we find intrinsic differences in the evolution of the stellar and gas mass fractions, BCG ages, and galaxy colour-magnitude diagrams, with gizmo-simba generally providing a good match to available data at z ≈ 0. gizmo-simba's unique black hole growth and feedback model yields agreement with the observed BH scaling relations at the intermediate-mass range and predicts a slightly different slope at high masses where few observations currently lie. Gizmo-Simba provides a new and novel platform to elucidate the co-evolution of galaxies, gas, and black holes within the densest cosmic environments
Databáze: OpenAIRE