68 citations · 171 across the 4 of their papers we have counts for
4 papers
Thermal Feedback in the high-mass star and cluster forming region W51
Adam Ginsburg, Ciriaco Goddi, J. M. Diederik Kruijssen +11
High-mass stars have generally been assumed to accrete most of their mass while already contracted onto the main sequence, but this hypothesis has not been observationally tested.…
Kinematic and Thermal Structure at the onset of high-mass star formation
S. Bihr, H. Beuther, H. Linz +6
We want to understand the kinematic and thermal properties of young massive gas clumps prior to and at the earliest evolutionary stages of high-mass star formation. Do we find sign…
The impact of thermodynamics on gravitational collapse: filament formation and magnetic field amplification
Thomas Peters, Dominik R. G. Schleicher, Ralf S. Klessen +4
Stars form by the gravitational collapse of interstellar gas. The thermodynamic response of the gas can be characterized by an effective equation of state. It determines how gas he…
The structure of molecular clouds and the universality of the clump mass function
Rowan J. Smith, Paul C. Clark, Ian A. Bonnell
Using an SPH simulation of a star-forming region in a molecular cloud, we show that the emergence of a clump mass function (CMF) resembling the stellar initial mass function (IMF)…