collaborators

5 papers

astro-ph.GA2026

The Small-scale Structures in the Wind of Messier 82

Yucheng Guo, Timothy Heckman, Sanchayeeta Borthakur +10

Small-scale multiphase structure plays a central role in galactic-wind evolution, yet the parsec-scale morphology and excitation of the warm ionised gas remain poorly constrained.…

astro-ph.GA2026

The Internal Nebular Attenuation Curve of Three-Dimensional Turbulent HII regions

Yifei Jin, Yong Shi, Ralph Sutherland +2

The internal dust attenuation of the Hii region reduces the observed emission-line fluxes. Turbulent density fields within each Hii region change the degree of the line-of-the-sigh…

astro-ph.GA2025

A Theoretical Three-Dimensional Diagram to Separate Star Formation, Active Galactic Nuclei, and Shocks in Galaxies

Peixin Zhu, Lisa J. Kewley, Ralph S. Sutherland +1

The excitation sources in galaxies are frequently mixed due to AGN and stellar feedback, including star formation, active galactic nuclei (AGNs), and shock excitation. Disentanglin…

astro-ph.GA2025

A model for the emission line galaxy luminosity function and flux ratios at high-redshifts

Aadarsh Pathak, J. Stuart B. Wyithe, Ralph S. Sutherland +1

We present emision line flux ratio predictions for galaxies at using the MAPPINGS V v5.2.0 photoionization modelling code combined with an analytic…

astro-ph.GA2025

Strong nebular HeII emission induced by He ionizing photons escaping through the clumpy winds of massive stars

Arpita Roy, Mark R. Krumholz, Stefania Salvadori +8

The origin of nebular HeII-emission in both local and high-redshift galaxies remains an unsolved problem. Various theories have been proposed to explain it, including HeII-ionizati…