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20062026
most citedMolecular Gas Properties on Cloud Scales Across the Local Star-forming Galaxy Population

153 citations · 636 across the 52 of their papers we have counts for

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Showing 2024Show all

6 papers · 1 filter

astro-ph.GA2024

CO isotopologue-derived molecular gas conditions and CO-to-H conversion factors in M51

Jakob den Brok, María J. Jiménez-Donaire, Adam Leroy +24

Over the past decade, several millimeter interferometer programs have mapped the nearby star-forming galaxy M51 at a spatial resolution of pc. This study combines observ…

astro-ph.GA2024

Molecular Hydrogen in the Extremely Metal-Poor, Star-Forming Galaxy Leo P

O. Grace Telford, Karin M. Sandstrom, Kristen B. W. McQuinn +4

The James Webb Space Telescope (JWST) has revealed unexpectedly rapid galaxy assembly in the early universe, in tension with models of star and galaxy formation. In the gas conditi…

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.GA2024★ 3 cited

A First-look at Spatially-resolved Infrared Supernova Remnants in M33 with JWST

Sumit K. Sarbadhicary, Erik Rosolowsky, Adam K. Leroy +12

We present the first spatially-resolved infrared images of supernova remnants (SNRs) in M33 with the unprecedented sensitivity and resolution of JWST. We analyze 40 SNRs in four JW…

astro-ph.GA2024★ 19 cited

PHANGS-MeerKAT and MHONGOOSE HI observations of nearby spiral galaxies: physical drivers of the molecular gas fraction,

Cosima Eibensteiner, Jiayi Sun, Frank Bigiel +36

The molecular-to-atomic gas ratio is crucial to the evolution of the interstellar medium in galaxies. We investigate the balance between the atomic () and molecular gas…

astro-ph.GA2024★ 29 cited

Redshift-dependent galaxy formation efficiency at in the FirstLight simulations

Daniel Ceverino, Yurina Nakazato, Naoki Yoshida +2

Current models of the formation of first galaxies predict low masses and faint objects at extremely high redshifts, z=9-15. However, the first observations of this epoch indicate a…