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astro-ph.GA2024
PHANGS-ML: the universal relation between PAH band and optical line ratios across nearby star-forming galaxies
Dalya Baron, Karin Sandstrom, Jessica Sutter +22
The structure and chemistry of the dusty interstellar medium (ISM) are shaped by complex processes that depend on the local radiation field, gas composition, and dust grain propert…
astro-ph.GA2021
Quenching, Mergers and Age Profiles for z=2 Galaxies in IllustrisTNG
Debosmita Pathak, Sirio Belli, Rainer Weinberger
Using the IllustrisTNG cosmological galaxy formation simulations, we analyze the physical properties of young quiescent galaxies at z=2 with stellar masses above 10^10.5 solar mass…