activity
20092026
most citedClouds, filaments and protostars: the Herschel Hi-GAL Milky Way

806 citations · 6.5k across the 135 of their papers we have counts for

collaborators
Showing 2017Show all

5 papers · 1 filter

astro-ph.GA2017★ 103 cited

The Physical Properties of Large-Scale Galactic Filaments

Catherine Zucker, Cara Battersby, Alyssa Goodman

The characterization of our Galaxy's longest filamentary gas features has been the subject of several studies in recent years, producing not only a sizeable sample of large-scale f…

astro-ph.GA2017★ 54 cited

Star formation in a high-pressure environment: An SMA view of the Galactic centre dust ridge

D. L. Walker, S. N. Longmore, Q. Zhang +14

The star formation rate in the Central Molecular Zone (CMZ) is an order of magnitude lower than predicted according to star formation relations that have been calibrated in the dis…

astro-ph.GA2017★ 44 cited

The Molecular Gas Environment in the 20 km s Cloud in the Central Molecular Zone

Xing Lu, Qizhou Zhang, Jens Kauffmann +9

We recently reported a population of protostellar candidates in the 20 km s cloud in the Central Molecular Zone of the Milky Way, traced by HO masers in gravitationally…

astro-ph.GA2017★ 31 cited

The Lifetimes of Phases in High-Mass Star-Forming Regions

Cara Battersby, John Bally, Brian Svoboda

High-mass stars form within star clusters from dense, molecular regions, but is the process of cluster formation slow and hydrostatic or quick and dynamic? We link the physical pro…

astro-ph.GA2017★ 32 cited

Origins of Scatter in the Relationship Between HCN 1-0 and Dense Gas Mass in the Galactic Center

E. A. C. Mills, C. Battersby

We investigate the correlation of HCN 1-0 with dense gas mass in the Galactic center. We find that in general (on the ~10 pc size scale of individual molecular cloud cores) HCN 1-0…