17 citations
Counting papers with at most 25 authors, so collaboration author lists do not stand in for the people here.
- University of ConnecticutUS5 papers
- California Institute of TechnologyUS4 papers
- CentraleSupélecFR3 papers
- Mathématiques et Informatique pour la Complexité et les Systèmes3 papers
- Pomona CollegeUS3 papers
- University of HullGB3 papers
- Korea Institute for Advanced StudyKR2 papers
- Université Paris-SaclayFR2 papers
- University of ManchesterGB2 papers
- Wesleyan CollegeUS2 papers
- Anna Needs Neuroblastoma AnswersUS1 paper
- Ben-Gurion University of the NegevIL1 paper
4 papers · 1 filter
Investigating black hole accretion and feedback self-regulation in Seyfert galaxies using the FIRE-3 cosmological hydrodynamic simulations
Jonathan Mercedes-Feliz, Daniel Anglés-Alcázar, Jose Cevallos +12
Recent observations of local Seyfert galaxies show an intriguing connection between Active Galactic Nuclei (AGN) luminosity and a deficit of molecular gas on ~50pc scales compared…
The role of galactic winds fueling central starbursts and quasars in the FIRE cosmological simulations
Jonathan Mercedes-Feliz, Daniel Anglés-Alcázar, Boon Kiat Oh +7
Central starbursts and Active Galactic Nuclei (AGN) are thought to be fueled by either galaxy interactions or secular processes in gravitationally unstable discs. We employ cosmolo…
Dense stellar clump formation driven by strong quasar winds in the FIRE cosmological hydrodynamic simulations
Jonathan Mercedes-Feliz, Daniel Anglés-Alcázar, Boon Kiat Oh +9
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 under the presen…
Why do Black Holes Trace Bulges (& Central Surface Densities), Instead of Galaxies as a Whole?
Philip F. Hopkins, Sarah Wellons, Daniel Angles-Alcazar +2
Previous studies of fueling black holes (BHs) in galactic nuclei have argued (on scales ~0.01-1000pc) accretion is dynamical with inflow rates $\dot{M}\simη\,M_{\rm gas}/t_{\rm dyn…