activity
20232026
most citedA nearly constant CN/HCN line ratio in nearby galaxies: CN as a new tracer of dense gas

9 citations · 9 across the 5 of their papers we have counts for

collaborators

5 papers

astro-ph.GA2026

EMBERS I: Low redshift post-starburst galaxies are frequently depleted in molecular gas relative to star forming progenitors

Ben F. Rasmussen, María Jesús Jiménez-Donaire, Sara L. Ellison +10

The cold gas content of post-starburst galaxies (PSBs) provides important insight into the mechanisms that drive rapid quenching, but a multiphase assessment of both the atomic and…

astro-ph.GA2025

SDSS-ALMA Legacy Value Archival Gas Exploration (SALVAGE) -- I: global star formation is governed by central (not global) molecular gas

Scott Wilkinson, Toby Brown, Chiara Circosta +3

Star-forming galaxies form tight relations between their stellar mass, star-formation rate, and molecular gas reservoir on global and resolved scales. On the path to quiescence, th…

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}…

astro-ph.GA2023

Stored in the archives: Uncovering the CN/CO intensity ratio with ALMA in nearby U/LIRGs

Blake Ledger, Toshiki Saito, Daisuke Iono +1

We present an archival Atacama Large Millimeter/submillimeter Array (ALMA) study of the CN N = 1 - 0 / CO J = 1 - 0 intensity ratio in nearby (z < 0.05) Ultra Luminous and Luminous…

astro-ph.GA2023★ 9 cited

A nearly constant CN/HCN line ratio in nearby galaxies: CN as a new tracer of dense gas

Christine D. Wilson, Ashley Bemis, Blake Ledger +1

We investigate the relationship between CN N = 1 - 0 and HCN J = 1 - 0 emission on scales from 30 pc to 400 pc using ALMA archival data, for which CN is often observed simultaneous…