activity
19952024
most citedWater in Star-Forming Regions with the Herschel Space Observatory (WISH): Overview of key program and first results

262 citations · 5.3k across the 88 of their papers we have counts for

collaborators
Showing 2019Show all

5 papers · 1 filter

astro-ph.SR2019★ 11 cited

Massive star formation via torus accretion: the effect of photoionization feedback

N. S. Sartorio, B. Vandenbroucke, D. Falceta-Goncalves +2

The formation of massive stars is a long standing problem. Although a number of theories of massive star formation exist, ideas appear to converge to a disk-mediated accretion scen…

astro-ph.SR2019★ 5 cited

Radiation hydrodynamic simulations of massive star formation via gravitationally trapped HII regions - Spherically symmetric ionised accretion flows

Kristin Lund, Kenneth Wood, Diego Falceta-Gonçalves +5

This paper investigates the gravitational trapping of HII regions predicted by steady-state analysis using radiation hydrodynamical simulations. We present idealised spherically sy…

astro-ph.SR2019★ 4 cited

Testing the stability of supersonic ionized Bondi accretion flows with radiation hydrodynamics

Bert Vandenbroucke, Nina S. Sartorio, Kenneth Wood +6

We investigate the general stability of 1D spherically symmetric ionized Bondi accretion onto a massive object in the specific context of accretion onto a young stellar object. We…

astro-ph.SR2019★ 72 cited

The central 1000 AU of a pre-stellar core revealed with ALMA. I. 1.3 mm continuum observations

Paola Caselli, Jaime E. Pineda, Bo Zhao +8

Stars like our Sun form in self-gravitating dense and cold structures within interstellar clouds, called pre-stellar cores. Although much is known about the physical structure of d…

astro-ph.GA2019★ 91 cited

The dynamical evolution of molecular clouds near the Galactic Centre - II. Spatial structure and kinematics of simulated clouds

J. M. D. Kruijssen, J. E. Dale, S. N. Longmore +16

The evolution of molecular clouds in galactic centres is thought to differ from that in galactic discs due to a significant influence of the external gravitational potential. We pr…