244 citations · 3.1k across the 55 of their papers we have counts for
56 papers
Star Cluster Formation in Clouds with Externally Driven Turbulence
Jamie D. Smith, James E. Dale, Sarah E. Jaffa +1
Star clusters are known to be formed in turbulent molecular clouds. How turbulence is driven in molecular clouds and what effect this has on star formation is still unclear. We com…
Collision Between Molecular Clouds-III: The effects of cloud initial density profile on head-on collisions
Tabassum S Tanvir, James E Dale
In this third paper in our cloud-collision series, we present the results from simulations of head-on collisions with a strongly centrally-condensed initial density profile of $\rm…
The complex multi-scale structure in simulated and observed emission maps of the proto-cluster cloud G0.253+0.016 (`the Brick')
Maya A. Petkova, J. M. Diederik Kruijssen, A. Louise Kluge +6
The Central Molecular Zone (CMZ; the central ~ 500 pc of the Milky Way) hosts molecular clouds in an extreme environment of strong shear, high gas pressure and density, and complex…
Galactic 26Al traces metal loss through hot chimneys
Martin G. H. Krause, Donna Rodgers-Lee, James E. Dale +2
Radioactive 26Al is an excellent tracer for metal ejection in the Milky Way, and can provide a direct constraint on the modelling of supernova feedback in galaxy evolution. Gamma-r…
Which feedback mechanisms dominate in the high-pressure environment of the Central Molecular Zone?
Ashley T. Barnes, Steven N. Longmore, James E. Dale +3
Supernovae (SNe) dominate the energy and momentum budget of stellar feedback, but the efficiency with which they couple to the interstellar medium (ISM) depends strongly on how eff…
Collision between Molecular Clouds I. The effect of the cloud virial ratio in head-on collisions
Tabassum S Tanvir, James E Dale
In a series of papers we investigate the effect of collisions between turbulent molecular clouds on their structure, evolution and star formation activity. In this paper we look in…