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