Zobrazeno 1 - 10
of 104
pro vyhledávání: '"Su, Kung Yi"'
Autor:
Su, Kung-Yi, Natarajan, Priyamvada, Cho, Hyerin, Narayan, Ramesh, Hopkins, Philip F., Anglés-Alcázar, Daniel, Prather, Ben S.
Coupling black hole (BH) feeding and feedback involves interactions across vast spatial and temporal scales that is computationally challenging. Tracking gas inflows and outflows from kilo-parsec scales to the event horizon for non-spinning BHs in th
Externí odkaz:
http://arxiv.org/abs/2410.13235
In an effort to understand the presence of super-virial gas detected in the Milky Way, we present our findings from isolated galaxy simulations of Milky Way-like systems using GIZMO with the FIRE-2 (Feedback In Realistic Environments) stellar feedbac
Externí odkaz:
http://arxiv.org/abs/2409.17252
The early growth of black holes (BHs) in atomic-cooling halos is likely influenced by feedback on the surrounding gas. While the effects of radiative feedback are well-documented, mechanical feedback, particularly from AGN jets, has been comparativel
Externí odkaz:
http://arxiv.org/abs/2409.12250
Autor:
Emami, Razieh, Hernquist, Lars, Smith, Randall, Steiner, James F., Tremblay, Grant, Finkbeiner, Douglas, Vogelsberger, Mark, Grindlay, Josh, Marinacci, Federico, Su, Kung-Yi, Garraffo, Cecilia, Ting, Yuan-Sen, Cargile, Phillip A., Davies, Rebecca L., Benton, Chloë E., Li, Yijia, Bugiani, Letizia, Khoram, Amir H., Bose, Sownak
We undertake a comprehensive investigation into the distribution of insitu stars within Milky Way-like galaxies, leveraging TNG50 simulations and comparing their predictions with data from the H3 survey. Our analysis reveals that 28% of galaxies demo
Externí odkaz:
http://arxiv.org/abs/2407.07169
Simulating accretion and feedback from the horizon scale of supermassive black holes (SMBHs) out to galactic scales is challenging because of the vast range of scales involved. Elaborating on \citet{Cho2023}, we describe and test a ``multi-zone'' tec
Externí odkaz:
http://arxiv.org/abs/2405.13887
Autor:
Qutob, Nadia, Emami, Razieh, Su, Kung-Yi, Smith, Randall, Hernquist, Lars, Triani, Dian P., Hummels, Cameron, Fielding, Drummond, Hopkins, Philip F., Somerville, Rachel S., Ballantyne, David R., Vogelsberger, Mark, Tremblay, Grant, Steiner, James F., Finkbeiner, Douglas, Narayan, Ramesh, Park, Minjung, Grindlay, Josh, Natarajan, Priyamvada, Hayward, Christopher C., Kereš, Dušan, Ponnada, Sam B., Belli, Sirio, Davies, Rebecca, Maheson, Gabriel, Bugiani, Letizia, Li, Yijia
We make an in-depth analysis of different AGN jet models' signatures, inducing quiescence in galaxies with a halo mass of $10^{12} M_\odot$. Three jet models, including cosmic ray-dominant, hot thermal, and precessing kinetic jets, are studied at two
Externí odkaz:
http://arxiv.org/abs/2312.14809
Autor:
Mercedes-Feliz, Jonathan, Anglés-Alcázar, Daniel, Oh, Boon Kiat, Hayward, Christopher C., Cochrane, Rachel K., Richings, Alexander J., Faucher-Giguère, Claude-André, Wellons, Sarah, Terrazas, Bryan A., Moreno, Jorge, Su, Kung Yi, Hopkins, Philip F.
We investigate the formation of dense stellar clumps in a suite of high-resolution cosmological zoom-in simulations of a massive, star forming galaxy at $z \sim 2$ under the presence of strong quasar winds. Our simulations include multi-phase ISM phy
Externí odkaz:
http://arxiv.org/abs/2310.19863
Autor:
Cho, Hyerin, Prather, Ben S., Narayan, Ramesh, Natarajan, Priyamvada, Su, Kung-Yi, Ricarte, Angelo, Chatterjee, Koushik
Fueling and feedback couple supermassive black holes (SMBHs) to their host galaxies across many orders of magnitude in spatial and temporal scales, making this problem notoriously challenging to simulate. We use a multi-zone computational method base
Externí odkaz:
http://arxiv.org/abs/2310.19135
Autor:
Su, Kung-Yi, Bryan, Greg L., Hayward, Christopher C., Somerville, Rachel S., Hopkins, Philip F., Emami, Razieh, Faucher-Giguère, Claude-André, Quataert, Eliot, Ponnada, Sam B., Fielding, Drummond, Kereš, Dušan
In the absence of supplementary heat, the radiative cooling of halo gas around massive galaxies (Milky Way mass and above) leads to an excess of cold gas or stars beyond observed levels. AGN jet-induced heating is likely essential, but the specific p
Externí odkaz:
http://arxiv.org/abs/2310.17692
Autor:
Hopkins, Philip F., Squire, Jonathan, Quataert, Eliot, Murray, Norman, Su, Kung-Yi, Steinwandel, Ulrich P., Kremer, Kyle, Faucher-Giguere, Claude-Andre, Wellons, Sarah
Recent numerical cosmological radiation-magnetohydrodynamic-thermochemical-star formation simulations have resolved the formation of quasar accretion disks with Eddington or super-Eddington accretion rates onto supermassive black holes (SMBHs) down t
Externí odkaz:
http://arxiv.org/abs/2310.04507