Zobrazeno 1 - 4
of 4
pro vyhledávání: '"Pellissier, Alisson"'
We present the Rhapsody-C simulations that extend the Rhapsody-G suite of massive galaxy clusters at the $M_{\rm vir}\sim10^{15}\thinspace{\rm M}_{\odot}$ scale with cosmological magneto-hydrodynamic zoom-in simulations that include anisotropic therm
Externí odkaz:
http://arxiv.org/abs/2301.02684
Autor:
Beckmann, Ricarda S., Dubois, Yohan, Pellissier, Alisson, Polles, Fiorella L., Olivares, Valeria
Publikováno v:
A&A 666, A71 (2022)
Centres of galaxy clusters must be efficiently reheated to avoid a cooling catastrophe. One potential reheating mechanism is anisotropic thermal conduction, which could transport thermal energy from intermediate radii to the cluster center. However,
Externí odkaz:
http://arxiv.org/abs/2204.12514
Autor:
Beckmann, Ricarda S., Dubois, Yohan, Pellissier, Alisson, Olivares, Valeria, Polles, Fiorella L., Hahn, Oliver, Guillard, Pierre, Lehnert, Matthew D.
Publikováno v:
A&A 665, A129 (2022)
One of the key physical processes that helps prevent strong cooling flows in galaxy clusters is the continued energy input from the central active galactic nucleus (AGN) of the cluster. However, it remains unclear how this energy is thermalised so th
Externí odkaz:
http://arxiv.org/abs/2204.03629
Autor:
Bouché, Nicolas F., Genel, Shy, Pellissier, Alisson, Dubois, Cédric, Contini, Thierry, Epinat, Benoît, Pillepich, Annalisa, Krajnović, Davor, Nelson, Dylan, Abril-Melgarejo, Valentina, Richard, Johan, Boogaard, Leindert A., Maseda, Michael, Mercier, Wilfried, Bacon, Roland, Steinmetz, Matthias, Vogelsberger, Mark
Publikováno v:
A&A 654, A49 (2021)
We investigate the specific angular momentum (sAM) $ j(
Externí odkaz:
http://arxiv.org/abs/2101.12250