activity
19952025
most citedRevealing the cold dust in low-metallicity environments: I - Photometry analysis of the Dwarf Galaxy Survey with Herschel

163 citations · 621 across the 15 of their papers we have counts for

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Showing astro-ph.GAShow all

8 papers · 1 filter

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}…

astro-ph.GA2024

Cloud-Scale Molecular Gas Properties of the Antennae Merger: A Comparative Study with PHANGS-ALMA Galaxies and NGC 3256

Nathan Brunetti, Christine D. Wilson, Hao He +8

We present observations of the central 9 kpc of the Antennae merger (NGC 4038/9) at 55 pc resolution in the CO 2-1 line obtained with the Atacama Large Millimeter/submillimeter Arr…

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.GA2018★ 110 cited

Comprehensive comparison of models for spectral energy distributions from 0.1 micron to 1 mm of nearby star-forming galaxies

L. K. Hunt, I. De Looze, M. Boquien +26

We have fit the far-ultraviolet (FUV) to sub-millimeter (850 micron) spectral energy distributions (SEDs) of the 61 galaxies from the "Key Insights on Nearby Galaxies: A Far-Infrar…

astro-ph.GA2014★ 68 cited

Extreme dust disks in Arp 220 as revealed by ALMA

C. D. Wilson, N. Rangwala, J. Glenn +3

We present new images of Arp 220 from the Atacama Large Millimeter/submillimeter Array with the highest combination of frequency (691 GHz) and resolution ($0.36 \times 0.20^{\prime…

astro-ph.GA2014★ 2 cited

A multiwavelength analysis of the clumpy FIR-bright sources in M33

G. Natale, K. Foyle, C. D. Wilson +1

We present a multiwavelength study of a sample of far-infrared (FIR) sources detected on the Herschel broad--band maps of the nearby galaxy M33. We perform source photometry on the…