Zobrazeno 1 - 8
of 8
pro vyhledávání: '"Clarke J Esmerian"'
Autor:
Clarke J. Esmerian, Nickolay Y. Gnedin
Publikováno v:
The Astrophysical Journal, Vol 968, Iss 2, p 113 (2024)
We model the interstellar dust content of the reionization era with a suite of cosmological, fluid-dynamical simulations of galaxies with stellar masses ranging from ∼10 ^5 to 10 ^9 M _⊙ in the first 1.2 Gyr of the Universe. We use a post-process
Externí odkaz:
https://doaj.org/article/33d1dbb395f24568aff975ca0e686af9
Autor:
Clarke J. Esmerian, Nickolay Y. Gnedin
Publikováno v:
The Astrophysical Journal, Vol 965, Iss 2, p 190 (2024)
Externí odkaz:
https://doaj.org/article/b3aef2e438f6415cabf26af3223e9b72
Autor:
Clarke J. Esmerian, Nickolay Y. Gnedin
Publikováno v:
The Astrophysical Journal, Vol 940, Iss 1, p 74 (2022)
We introduce a model for the explicit evolution of interstellar dust in a cosmological galaxy formation simulation. We post-process a simulation from the Cosmic Reionization on Computers project, integrating an ordinary differential equation for the
Externí odkaz:
https://doaj.org/article/9da91ed6d08c47818f6a3da0e788f7f2
Autor:
Yue Pan, Christine M Simpson, Andrey Kravtsov, Facundo A Gómez, Robert J J Grand, Federico Marinacci, Rüdiger Pakmor, Viraj Manwadkar, Clarke J Esmerian
We use the Auriga simulations to probe different satellite quenching mechanisms operating at different mass scales ($10^5 M_\odot \lesssim M_\star \lesssim 10^{11} M_\odot$) in Milky Way-like hosts. Our goal is to understand the origin of the satelli
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::099f5b3da4854f86874cc5e67993c355
http://arxiv.org/abs/2208.13805
http://arxiv.org/abs/2208.13805
Autor:
Zachary Hafen, Claude André Faucher-Giguère, Andrew Wetzel, Eliot Quataert, Clarke J. Esmerian, Andrey V. Kravtsov, Dušan Kereš, Jonathan Stern
We examine the thermodynamic state and cooling of the low-$z$ Circum-Galactic Medium (CGM) in five FIRE-2 galaxy formation simulations of Milky Way-mass galaxies. We find that the CGM in these simulations is generally multiphase and dynamic, with a w
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::5335017835fbcf7b82f05027dd3fa9c2
Autor:
Clarke J. Esmerian, Nickolay Y. Gnedin
Several massive ($M_{*} > 10^8 M_{\odot}$), high-redshift ($z = 8-10$) galaxies have recently been discovered to contain stars with ages of several hundred million years, pushing the onset of star formation in these galaxies back to $z\sim15$. The ve
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::f0e3307fd789f9501e20b61eb9e54217
Autor:
Claude André Faucher-Giguère, Kareem El-Badry, Andrew Wetzel, Zachary Hafen, T. K. Chan, Daniel Anglés-Alcázar, Clarke J. Esmerian, Shea Garrison-Kimmel, Cameron Hummels, Dušan Kereš, Philip F. Hopkins, Norman Murray, Jonathan Stern
Publikováno v:
Monthly Notices of the Royal Astronomical Society, vol 494, iss 3
We analyze the different fates of the circumgalactic medium (CGM) in FIRE-2 cosmological simulations, focusing on the redshifts z=0.25 and z=2 representative of recent surveys. Our analysis includes 21 zoom-in simulations covering the halo mass range
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::4c87fcb92158d69976a524c9dc297cd8
Autor:
Nickolay Y. Gnedin, Clarke J. Esmerian
Publikováno v:
The Astrophysical Journal. 912:166
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::5d4cfe26db194a04114fcd1cbb1edc4c
https://doi.org/10.3847/1538-4357/abfa94
https://doi.org/10.3847/1538-4357/abfa94