11 citations · 17 across the 6 of their papers we have counts for
7 papers
Toward Resolution Convergence for Star Formation and Galactic Winds in Galaxy Simulations
Xue-Fu Li, Weishan Zhu, Tian-Rui Wang +2
The predictive power of hydrodynamic simulations of galaxies is often hampered by the resolution dependence of sub-grid models for star formation (SF) and stellar feedback. We pres…
Properties of Galactic Outflows Driven by Starburst at Cosmic Noon: Insights from Hydrodynamical Simulations
Huan Chen, Weishan Zhu, Xue-Fu Li +3
We investigate starburst-driven galactic outflows in low-mass galaxies () at cosmic noon using high-resolution 3D hydrodynamical simulations based o…
The Quasar Proximity Effect as an Alternative Probe of Quasar Pair Distances
Huanqing Chen, Camille Avestruz, Jakob Wiest
Recently discovered quasar pairs at high redshifts (5) are likely precursors to supermassive black hole mergers, providing a promising window to high redshift quasar grow…
Cosmic Reionization On Computers: Biases and Uncertainties in the Measured Mean Free Path at the End Stage of Reionization
Huanqing Chen, Jiawen Fan, Camille Avestruz
Recent observations and analyses of absorption in quasar spectra suggest a rapid drop in the mean free path (MFP) at the late stage of reionization at . We use the Cosmic R…
Cosmic Reionization on Computers: The Evolution of Ionizing Background and Mean Free Path
Jiawen Fan, Huanqing Chen, Camille Avestruz +1
Observations of the end stages of reionization indicate that at , the ionizing background is not uniform and the mean free path (MFP) changes drastically. As MFP is c…
Learning Reionization History from Quasars with Simulation-Based Inference
Huanqing Chen, Joshua Speagle, Keir K. Rogers
Understanding the entire history of the ionization state of the intergalactic medium (IGM) is at the frontier of astrophysics and cosmology. A promising method to achieve this is b…
The Green Bank Ammonia Survey: Unveiling the Dynamics of the Barnard 59 star-forming Clump
E. Redaelli, F. O. Alves, P. Caselli +17
Understanding the early stages of star formation is a research field of ongoing development, both theoretically and observationally. In this context, molecular data have been conti…