3 papers
astro-ph.GA2025
MAUVE-MUSE: A Star Formation-driven Outflow Caught in the Act of Quenching the Stripped Virgo Galaxy NGC 4064
Amy Attwater, Barbara Catinella, Luca Cortese +10
The rapid quenching of satellite galaxies in dense environments is often attributed to environmental processes such as ram pressure stripping. However, stripping alone cannot fully…
astro-ph.GA2025
Increased molecular gas velocity dispersion and star formation efficiency in barred galaxy centres
Jennifer M. Laing, Christine D. Wilson
Work by the Physics at High Angular resolution in Nearby GalaxieS (PHANGS) collaboration found higher molecular gas surface densities and velocity dispersions in the centres of bar…
astro-ph.GA2025
Building on the archives: Connecting the CN/CO intensity ratio with global galaxy properties in nearby U/LIRGs
Blake Ledger, Christine D. Wilson, Osvald Klimi +2
We use the CN/CO intensity ratio to obtain the dense gas fraction, , for a sample of 16 Ultra-luminous and Luminous Infrared Galaxies and compare $f_{\text{dense}…