activity
20182026
most citedOn the Survival of Cool Clouds in the Circum-Galactic Medium

117 citations · 382 across the 17 of their papers we have counts for

collaborators

17 papers

astro-ph.GA2026

Resonantly Scattered CIV Emission in Local Star-forming Galaxies: Radiative Transfer Constraints on High-ionization Gas in Reionization Analogs

Zhihui Li, Danielle A. Berg, Simon Gazagnes +4

Rest-frame ultraviolet emission lines are diagnostics of hard ionizing spectra and highly ionized gas in galaxies resembling the sources of cosmic reionization. Nebular CIV emissio…

astro-ph.GA2026

The Prevalence of Turbulence-Regulated Multiphase Galactic Winds in Star-Forming Galaxies

Zhihui Li, Timothy Heckman, Max Gronke +8

We build upon our previously developed multi-ion radiative transfer (RT) framework, PEACOCK, to investigate the kinematic and energetic structure of cool-to-warm galactic winds in…

astro-ph.GA2026

Kinematically Coherent Multiphase Galactic Winds in Star-Forming Galaxies Revealed by Unified Radiative Transfer Modeling of UV Emission and Absorption Lines

Zhihui Li, Timothy Heckman, Max Gronke +8

We present PEACOCK, a three-dimensional Monte Carlo radiative transfer (RT) framework designed to self-consistently model rest-frame ultraviolet emission and absorption lines arisi…

astro-ph.GA2026

BLUEPRINT: Blue-dominant Lyman- emission as evidence of gas inflow in ultra-low-mass galaxies at z = 3

Tamal Mukherjee, Zhihui Li, Tayyaba Zafar +4

We report the detection of a clumpy, blue-dominated Ly emission at z = 3.066 located in the heart of a cosmic web filament in the MUSE eXtremely Deep Field (MXDF), spatially ass…

astro-ph.GA2024

Synergistic Radiative Transfer Modeling of MgII and Lyα Emission in Multiphase, Clumpy Galactic Environments: Application to Low-Redshift Lyman Continuum Leakers

Zhihui Li, Max Gronke, Timothy Heckman +9

We conducted systematic radiative transfer (RT) modeling of the Mg II doublet line profiles for 33 low-redshift Lyman continuum (LyC) leakers, and Ly modeling for a subset of si…

astro-ph.GA2024★ 2 cited

Gas Accretion Traced by Blue-Dominated Ly Emission and Redshifted UV Absorption Lines in Protocluster Galaxies at z = 2.3 from the KBSS-KCWI Survey

Claire Bolda, Zhihui Li, Dawn K. Erb +2

Ly emission with a dominant blueshifted peak can probe gas flowing through the circumgalactic medium as it accretes onto galaxies and fuels new star formation, although it has s…

astro-ph.GA2023★ 2 cited

ALPACA: A New Semi-Analytic Model for Metal Absorption Lines Emerging from Clumpy Galactic Environments

Zhihui Li, Max Gronke, Charles Steidel

We present a new semi-analytic formalism for modeling metal absorption lines that emerge from a clumpy galactic environment, ALPACA. We predict the ''down-the-barrel'' (DTB) metal…

astro-ph.GA2022★ 29 cited

The Circumgalactic Medium of Extreme Emission Line Galaxies at z ~ 2: Resolved Spectroscopy and Radiative Transfer Modeling of Spatially Extended Lyman-alpha Emission in the KBSS-KCWI Survey

Dawn K. Erb, Zhihui Li, Charles C. Steidel +5

The resonantly scattered Lyman- line illuminates the extended halos of neutral hydrogen in the circumgalactic medium of galaxies. We present integral field Keck Cosmic Web Image…

astro-ph.GA2021

Deciphering the Lyman- Emission Line: Towards the Understanding of Galactic Properties Extracted from Ly Spectra via Radiative Transfer Modeling

Zhihui Li, Max Gronke

Existing ubiquitously in the Universe with the highest luminosity, the Lyman- emission line encodes abundant physical information about the gaseous medium it interacts with. Nev…

astro-ph.GA2021★ 18 cited

Where Outflows Meet Inflows: Gas Kinematics in SSA22 Lyman- Blob 2 Decoded by Advanced Radiative Transfer Modelling

Zhihui Li, Charles C. Steidel, Max Gronke +2

We present new spectroscopic observations of Lyman- (Ly) Blob 2 ( 3.1). We observed extended Ly emission in three distinct regions, where the highest Ly surface…

astro-ph.GA2021★ 41 cited

The KBSS-KCWI Survey: The connection between extended Ly halos and galaxy azimuthal angle at

Yuguang Chen, Charles C. Steidel, Dawn K. Erb +9

We present the first statistical analysis of kinematically-resolved, spatially-extended Ly emission around galaxies in the Keck Baryonic Structure Survey (KBSS) using…

astro-ph.GA2020★ 24 cited

Revisiting the Gas Kinematics in SSA22 Lyman- Blob 1 with Radiative Transfer Modeling in a Multiphase, Clumpy Medium

Zhihui Li, Charles C. Steidel, Max Gronke +1

We present new observations of Lyman- (Ly) Blob 1 (LAB1) in the SSA22 protocluster region ( = 3.09) using the Keck Cosmic Web Imager (KCWI) and the Keck Multi-object Spect…

astro-ph.HE2020★ 62 cited

SN2019dge: a Helium-rich Ultra-Stripped Envelope Supernova

Yuhan Yao, Kishalay De, Mansi M. Kasliwal +28

We present observations of ZTF18abfcmjw (SN2019dge), a helium-rich supernova with a fast-evolving light curve indicating an extremely low ejecta mass () and l…

astro-ph.GA2019★ 117 cited

On the Survival of Cool Clouds in the Circum-Galactic Medium

Zhihui Li, Philip F. Hopkins, Jonathan Squire +1

We explore the survival of cool clouds in multi-phase circum-galactic media. We revisit the "cloud crushing problem" in a large survey of simulations including radiative cooling, s…

astro-ph.GA2019★ 33 cited

The Evolution of the Interstellar Medium in Post-Starburst Galaxies

Zhihui Li, K. Decker French, Ann I. Zabludoff +1

We derive dust masses () from the spectral energy distributions of 58 post-starburst galaxies (PSBs). There is an anticorrelation between specific dust mass ($M_{\rm…

astro-ph.GA2018★ 47 cited

Interstellar Medium and Star Formation of Starburst Galaxies on the Merger Sequence

Jinyi Shangguan, Luis C. Ho, Ruancun Li +3

The interstellar medium is a key ingredient that governs star formation in galaxies. We present a detailed study of the infrared (~ 1-500 micron) spectral energy distributions of a…

astro-ph.GA2018★ 7 cited

Extreme [OIII] Emitters at z 0.5

Zhihui Li, Matthew A. Malkan

We have found a sample of extreme emission-line galaxies (EELGs) with strong [OIII]5007 emission at z 0.5. Using broadband photometric selection and requiring small uncer…