activity
20062023
most citedDense gas in the Galactic central molecular zone is warm and heated by turbulence

234 citations · 2.4k across the 50 of their papers we have counts for

collaborators

50 papers

astro-ph.GA2023★ 6 cited

The JWST Galactic Center Survey -- A White Paper

Rainer Schoedel, Steve Longmore, Jonny Henshaw +111

The inner hundred parsecs of the Milky Way hosts the nearest supermassive black hole, largest reservoir of dense gas, greatest stellar density, hundreds of massive main and post ma…

astro-ph.GA2023★ 1 cited

Widespread Hot Ammonia in the Central Kiloparsec of the Milky Way

Tierra M. Candelaria, E. A. C Mills, David S. Meier +2

The inner 300-500 pc of the Milky Way has some of the most extreme gas conditions in our Galaxy. Physical properties of the Central Molecular Zone (CMZ), including temperature, den…

astro-ph.GA2023★ 7 cited

CMZoom III: Spectral Line Data Release

Daniel Callanan, Steven N. Longmore, Cara Battersby +21

We present an overview and data release of the spectral line component of the SMA Large Program, \textit{CMZoom}. \textit{CMZoom} observed CO(2-1), CO(2-1) and C$^{18…

astro-ph.GA2022★ 14 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.GA2022★ 32 cited

The Morpho-Kinematic Architecture of Super Star Clusters in the Center of NGC253

Rebecca C. Levy, Alberto D. Bolatto, Adam K. Leroy +9

The center of the nearby galaxy NGC\,253 hosts a population of more than a dozen super star clusters (SSCs) which are still in the process of forming. The majority of the star form…

astro-ph.GA2022★ 8 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…