118 citations · 379 across the 5 of their papers we have counts for
5 papers
Tracing the Conversion of Gas into Stars in Young Massive Cluster Progenitors
D. L. Walker, S. N. Longmore, N. Bastian +5
Whilst young massive clusters (YMCs; 10 M, age 100 Myr) have been identified in significant numbers, their progenitor gas clouds have elude…
A cluster in the making: ALMA reveals the initial conditions for high-mass cluster formation
J. M. Rathborne, S. N. Longmore, J. M. Jackson +9
G0.253+0.016 is a molecular clump that appears to be on the verge of forming a high mass, Arches-like cluster. Here we present new ALMA observations of its small-scale (~0.07 pc) 3…
Absorption Filaments Towards the Massive Clump G0.253+0.016
John Bally, J. M. Rathborne, S. N. Longmore +11
ALMA HCO+ observations of the infrared dark cloud G0.253+0.016 located in the Central Molecular Zone of the Galaxy are presented. The 89 GHz emission is area-filling, optically thi…
Turbulence sets the initial conditions for star formation in high-pressure environments
J. M. Rathborne, S. N. Longmore, J. M. Jackson +9
Despite the simplicity of theoretical models of supersonically turbulent, isothermal media, their predictions successfully match the observed gas structure and star formation activ…
Low EUV Luminosities Impinging on Protoplanetary Disks
I. Pascucci, L. Ricci, U. Gorti +4
The amount of high-energy stellar radiation reaching the surface of protoplanetary disks is essential to determine their chemistry and physical evolution. Here, we use millimetric…