Zobrazeno 1 - 10
of 699
pro vyhledávání: '"Chan, T. K"'
Autor:
Wetzel, Andrew, Hayward, Christopher C., Sanderson, Robyn E., Ma, Xiangcheng, Angles-Alcazar, Daniel, Feldmann, Robert, Chan, T. K, El-Badry, Kareem, Wheeler, Coral, Garrison-Kimmel, Shea, Nikakhtar, Farnik, Panithanpaisal, Nondh, Arora, Arpit, Gurvich, Alexander B., Samuel, Jenna, Sameie, Omid, Pandya, Viraj, Hafen, Zachary, Hummels, Cameron, Loebman, Sarah, Boylan-Kolchin, Michael, Bullock, James S., Faucher-Giguere, Claude-Andre, Keres, Dusan, Quataert, Eliot, Hopkins, Philip F.
We describe a public data release of the FIRE-2 cosmological zoom-in simulations of galaxy formation, available at http://flathub.flatironinstitute.org/fire, from the Feedback In Realistic Environments (FIRE) project. FIRE-2 simulations achieve parse
Externí odkaz:
http://arxiv.org/abs/2202.06969
Autor:
Hafen, Zachary, Stern, Jonathan, Bullock, James, Gurvich, Alex B., Yu, Sijie, Faucher-Giguere, Claude-Andre, Fielding, Drummond B., Angles-Alcazar, Daniel, Quataert, Eliot, Wetzel, Andrew, Starkenburg, Tjitske, Boylan-Kolchin, Michael, Moreno, Jorge, Feldmann, Robert, El-Badry, Kareem, Chan, T. K., Trapp, Cameron, Keres, Dusan, Hopkins, Philip F.
We use FIRE simulations to study disk formation in z~0, Milky Way-mass galaxies, and conclude that a key ingredient for the formation of thin stellar disks is the ability for accreting gas to develop an aligned angular momentum distribution via inter
Externí odkaz:
http://arxiv.org/abs/2201.07235
Autor:
Chan, T. K., Keres, Dusan, Gurvich, Alexander B., Hopkins, Philip, Trapp, Cameron, Ji, Suoqing, Faucher-Giguere, Claude-Andre
Cosmic rays (CRs) are an important component in the interstellar medium (ISM), but their effect on the dynamics of the disk-halo interface (< 10 kpc from the disk) is still unclear. We study the influence of CRs on the gas above the disk with high-re
Externí odkaz:
http://arxiv.org/abs/2110.06231
Autor:
Kado-Fong, Erin, Sanderson, Robyn E., Greene, Jenny E., Cunningham, Emily C., Wheeler, Coral, Chan, T. K., El-Badry, Kareem, Hopkins, Philip F., Wetzel, Andrew, Boylan-Kolchin, Michael, Faucher-Giguère, Claude-André, Huang, Song, Quataert, Eliot, Starkenburg, Tjitske
Extended, old, and round stellar halos appear to be ubiquitous around high-mass dwarf galaxies ($10^{8.5}
Externí odkaz:
http://arxiv.org/abs/2109.05034
Autor:
Trapp, Cameron, Keres, Dusan, Chan, T. K., Escala, Ivanna, Hummels, Cameron, Hopkins, Philip F., Faucher-Giguere, Claude-Andre, Murray, Norman, Quataert, Eliot, Wetzel, Andrew
Publikováno v:
2022MNRAS.509.4149T
Observations indicate that a continuous supply of gas is needed to maintain observed star formation rates in large, disky galaxies. To fuel star formation, gas must reach the inner regions of such galaxies. Despite its crucial importance for galaxy e
Externí odkaz:
http://arxiv.org/abs/2105.11472
We present a new radiative transfer method (SPH-M1RT) that is coupled dynamically with smoothed particle hydrodynamics (SPH). We implement it in the (task-based parallel) SWIFT galaxy simulation code but it can be straightforwardly implemented in oth
Externí odkaz:
http://arxiv.org/abs/2102.08404
Autor:
Su, Kung-Yi, Hopkins, Philip F., Bryan, Greg L., Somerville, Rachel S., Hayward, Christopher C., Anglés-Alcázar, Daniel, Faucher-Giguère, Claude-André, Wellons, Sarah, Stern, Jonathan, Terrazas, Bryan A., Chan, T. K., Orr, Matthew E., Hummels, Cameron, Feldmann, Robert, Kereš, Dušan
Without additional heating, radiative cooling of gas in the halos of massive galaxies (Milky Way and above) produces cold gas or stars in excess of that observed. Previous work suggested that AGN jets are likely required, but the form of jet energy r
Externí odkaz:
http://arxiv.org/abs/2102.02206
Autor:
Ji, Suoqing, Kereš, Dušan, Chan, T. K., Stern, Jonathan, Hummels, Cameron B., Hopkins, Philip F., Quataert, Eliot, Faucher-Giguère, Claude-André
We study the impact of cosmic rays (CRs) on the structure of virial shocks, using a large suite of high-resolution cosmological FIRE-2 simulations accounting for CR injection by supernovae. In massive ($M_{\rm halo} \gtrsim 10^{11}\,M_{\odot}$), low-
Externí odkaz:
http://arxiv.org/abs/2011.04706
Autor:
Stern, Jonathan, Faucher-Giguère, Claude-André, Fielding, Drummond, Quataert, Eliot, Hafen, Zachary, Gurvich, Alexander B., Ma, Xiangcheng, Byrne, Lindsey, El-Badry, Kareem, Anglés-Alcázar, Daniel, Chan, T. K., Feldmann, Robert, Kereš, Dušan, Wetzel, Andrew, Murray, Norman, Hopkins, Philip F.
We use the FIRE-2 cosmological simulations to study the formation of a quasi-static, virial-temperature gas phase in the circumgalactic medium (CGM) at redshifts 0
Externí odkaz:
http://arxiv.org/abs/2006.13976
Autor:
Gurvich, Alexander B., Faucher-Giguère, Claude-André, Richings, Alexander J., Hopkins, Philip F., Grudić, Michael Y., Hafen, Zachary, Wellons, Sarah, Stern, Jonathan, Quataert, Eliot, Chan, T. K., Orr, Matthew E., Kereš, Dušan, Wetzel, Andrew, Hayward, Christopher C., Loebman, Sarah R., Murray, Norman
Pressure balance plays a central role in models of the interstellar medium (ISM), but whether and how pressure balance is realized in a realistic multiphase ISM is not yet well understood. We address this question using a set of FIRE-2 cosmological z
Externí odkaz:
http://arxiv.org/abs/2005.12916