activity
20162026
most citedNew Constraints on the CO(2-1)/(1-0) Line Ratio Across Nearby Disc Galaxies

130 citations · 1.3k across the 66 of their papers we have counts for

collaborators
Showing 2022Show all

8 papers · 1 filter

astro-ph.GA20221 cited

PHANGS-JWST First Results: Dust embedded star clusters in NGC 7496 selected via 3.3 m PAH emission

Jimena Rodriguez, Janice Lee, Bradley Whitmore +38

The earliest stages of star formation occur enshrouded in dust and are not observable in the optical. Here we leverage the extraordinary new high-resolution infrared imaging from J…

astro-ph.GA202214 cited

ALMA uncovers highly filamentary structure towards the Sgr E region

J. Wallace, C. Battersby, E. A. C. Mills +7

We report on the discovery of linear filaments observed in CO(1-0) emission for a field of view toward the Sgr E star forming region centered at (l,b)=(358.720, 0.…

astro-ph.GA20228 cited

The initial conditions for young massive cluster formation in the Galactic Centre: convergence of large-scale gas flows

Bethan A. Williams, Daniel L. Walker, Steven N. Longmore +12

Young massive clusters (YMCs) are compact (1 pc), high-mass (>10 M) stellar systems of significant scientific interest. Due to their rarity and rapid fo…

astro-ph.GA2022

Star Formation in the Central Molecular Zone of the Milky Way

Jonathan D. Henshaw, Ashley T. Barnes, Cara Battersby +3

The Central Molecular Zone (CMZ) is a ring-like accumulation of molecular gas in the innermost few hundred parsecs of the Milky Way, generated by the inward transport of matter dri…

astro-ph.GA202233 cited

Planetary Nebula Luminosity Function distances for 19 galaxies observed by PHANGS-MUSE

Fabian Scheuermann, Kathryn Kreckel, Gagandeep S. Anand +15

We provide new planetary nebula luminosity function (PNLF) distances to 19 nearby spiral galaxies that were observed with VLT/MUSE by the PHANGS collaboration. Emission line ratios…

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…