806 citations · 6.5k across the 135 of their papers we have counts for
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A Brief Update on the CMZoom Survey
Cara Battersby, Eric Keto, Qizhou Zhang +16
The inner few hundred parsecs of the Milky Way, the Central Molecular Zone (CMZ), is our closest laboratory for understanding star formation in the extreme environments (hot, dense…
Star formation rates on global and cloud scales within the Galactic Centre
Ashley Thomas Barnes, Steven Longmore, Cara Battersby +2
The environment within the inner few hundred parsecs of the Milky Way, known as the "Central Molecular Zone" (CMZ), harbours densities and pressures orders of magnitude higher than…
Deeply Embedded Protostellar Population in the Central Molecular Zone Suggested by HO Masers and Dense Cores
Xing Lu, Qizhou Zhang, Jens Kauffmann +4
The Central Molecular Zone (CMZ), usually referring to the inner 500 pc of the Galaxy, contains a dozen of massive ( ) molecular clouds. Are these clouds going t…
Toward gas exhaustion in the W51 high-mass protoclusters
Adam Ginsburg, W. M. Goss, Ciriaco Goddi +10
We present new JVLA observations of the high-mass cluster-forming region W51A from 2 to 16 GHz with resolution 0.3 - 0.5". The data reveal a wealth of observatio…
Molecular gas kinematics within the central 250 pc of the Milky Way
J. D. Henshaw, S. N. Longmore, J. M. D. Kruijssen +23
Using spectral-line observations of HNCO, N2H+, and HNC, we investigate the kinematics of dense gas in the central ~250 pc of the Galaxy. We present SCOUSE (Semi-automated multi-CO…
Using young massive star clusters to understand star formation and feedback in high-redshift-like environments
Steven Longmore, Ashley Barnes, Cara Battersby +9
The formation environment of stars in massive stellar clusters is similar to the environment of stars forming in galaxies at a redshift of 1 - 3, at the peak star formation rate de…