activity
20162023
most citedNew Constraints on the CO(2-1)/(1-0) Line Ratio Across Nearby Disc Galaxies

130 citations · 410 across the 10 of their papers we have counts for

collaborators

16 papers

astro-ph.GA202227 cited

A 2-3 mm high-resolution molecular line survey towards the centre of the nearby spiral galaxy NGC 6946

Cosima Eibensteiner, Ashley T. Barnes, Frank Bigiel +30

The complex physical, kinematic, and chemical properties of galaxy centres make them interesting environments to examine with molecular line emission. We present new " (${\sim…

astro-ph.GA202168 cited

VERTICO: The Virgo Environment Traced In CO Survey

Toby Brown, Christine D. Wilson, Nikki Zabel +33

We present the Virgo Environment Traced in CO (VERTICO) survey, a new effort to map CO(), CO(), and CO() in 51 Virgo Cluster galaxies with the A…

astro-ph.GA202137 cited

Dense molecular gas properties on 100 pc scales across the disc of NGC 3627

I. Bešlić, A. T. Barnes, F. Bigiel +29

It is still poorly constrained how the densest phase of the interstellar medium varies across galactic environment. A large observing time is required to recover significant emissi…

astro-ph.GA2021130 cited

New Constraints on the CO(2-1)/(1-0) Line Ratio Across Nearby Disc Galaxies

J. S. den Brok, D. Chatzigiannakis, F. Bigiel +18

Both the CO(2-1) and CO(1-0) lines are used to trace the mass of molecular gas in galaxies. Translating the molecular gas mass estimates between studies using different lines requi…

astro-ph.EP20208 cited

A Dust Trap in the Young Multiple System HD 34700

Peyton Benac, Luca Matra, David J. Wilner +6

Millimeter observations of disks around young stars reveal substructures indicative of gas pressure traps that may aid grain growth and planet formation. We present Submillimeter A…

astro-ph.GA2020

Dynamical Equilibrium in the Molecular ISM in 28 Nearby Star-Forming Galaxies

Jiayi Sun, Adam K. Leroy, Eve C. Ostriker +26

We compare the observed turbulent pressure in molecular gas, , to the required pressure for the interstellar gas to stay in equilibrium in the gravitational potent…