Zobrazeno 1 - 10
of 398
pro vyhledávání: '"Booth, C. M."'
Akademický článek
Tento výsledek nelze pro nepřihlášené uživatele zobrazit.
K zobrazení výsledku je třeba se přihlásit.
K zobrazení výsledku je třeba se přihlásit.
Autor:
Schaye, Joop, Crain, Robert A., Bower, Richard G., Furlong, Michelle, Schaller, Matthieu, Theuns, Tom, Vecchia, Claudio Dalla, Frenk, Carlos S., McCarthy, I. G., Helly, John C., Jenkins, Adrian, Rosas-Guevara, Y. M., White, Simon D. M., Baes, Maarten, Booth, C. M., Camps, Peter, Navarro, Julio F., Qu, Yan, Rahmati, Alireza, Sawala, Till, Thomas, Peter A., Trayford, James
Publikováno v:
2015, MNRAS, 446, 521
We introduce the Virgo Consortium's EAGLE project, a suite of hydrodynamical simulations that follow the formation of galaxies and black holes in representative volumes. We discuss the limitations of such simulations in light of their finite resoluti
Externí odkaz:
http://arxiv.org/abs/1407.7040
Akademický článek
Tento výsledek nelze pro nepřihlášené uživatele zobrazit.
K zobrazení výsledku je třeba se přihlásit.
K zobrazení výsledku je třeba se přihlásit.
Autor:
Rosas-Guevara, Y. M., Bower, R. G., Schaye, J., Furlong, M., Frenk, C. S., Booth, C. M., Crain, R., Vecchia, C. Dalla, Schaller, M., Theuns, T.
Feedback from energy liberated by gas accretion onto black holes (BHs) is an attractive mechanism to explain the exponential cut-off at the massive end of the galaxy stellar mass function (SMF). Semi-analytic models of galaxy formation in which this
Externí odkaz:
http://arxiv.org/abs/1312.0598
The observed clustering of galaxies and the cross-correlation of galaxies and mass provide important constraints on both cosmology and models of galaxy formation. Even though the dissipation and feedback processes associated with galaxy formation are
Externí odkaz:
http://arxiv.org/abs/1310.7571
Publikováno v:
ApJL 777, L16, 2013
We present results from high-resolution hydrodynamic simulations of isolated SMC- and Milky Way-sized galaxies that include a model for feedback from galactic cosmic rays (CRs). We find that CRs are naturally able to drive winds with mass loading fac
Externí odkaz:
http://arxiv.org/abs/1308.4974
We compute the z = 3 neutral hydrogen column density distribution function f(NHI) for 19 simulations drawn from the OWLS project using a post-processing correction for self-shielding calculated with full radiative transfer of the ionising background
Externí odkaz:
http://arxiv.org/abs/1307.6879
Autor:
Haas, Marcel R., Schaye, Joop, Booth, C. M., Vecchia, Claudio Dalla, Springel, Volker, Theuns, Tom, Wiersma, Robert P. C.
We use hydrodynamical simulations from the OWLS project to investigate the dependence of the physical properties of galaxy populations at redshift 2 on the assumed star formation law, the equation of state imposed on the unresolved interstellar mediu
Externí odkaz:
http://arxiv.org/abs/1211.3120
Autor:
Haas, Marcel R., Schaye, Joop, Booth, C. M., Vecchia, Claudio Dalla, Springel, Volker, Theuns, Tom, Wiersma, Robert P. C.
We use hydrodynamical simulations from the OWLS project to investigate the dependence of the physical properties of galaxy populations at redshift 2 on metal-line cooling and feedback from star formation and active galactic nuclei (AGN). We find that
Externí odkaz:
http://arxiv.org/abs/1211.1021
We use numerical simulations to investigate how the statistical properties of dark matter (DM) haloes are affected by the baryonic processes associated with galaxy formation. We focus on how these processes influence the spin and shape of a large num
Externí odkaz:
http://arxiv.org/abs/1207.4555