163 citations · 894 across the 21 of their papers we have counts for
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Accretion driven turbulence in filaments II: Effects of self-gravity
Stefan Heigl, Matthias Gritschneder, Andreas Burkert
We extend our previous work on simulations with the code RAMSES on accretion driven turbulence by including self-gravity and study the effects of core formation and collapse. We sh…
Carina's Pillars of Destruction: the view from ALMA
P. D. Klaassen, M. R. Reiter, A. F. McLeod +3
Forming high-mass stars have a significant effect on their natal environment. Their feedback pathways, including winds, outflows, and ionising radiation, shape the evolution of the…
Morphology of prestellar cores in pressure confined filaments
Stefan Heigl, Matthias Gritschneder, Andreas Burkert
Observations of prestellar cores in star-forming filaments show two distinct morphologies. While molecular line measurements often show broad cores, submillimeter continuum observa…
Accretion driven turbulence in filaments I: Non-gravitational accretion
Stefan Heigl, Andreas Burkert, Matthias Gritschneder
We study accretion driven turbulence for different inflow velocities in star forming filaments using the code ramses. Filaments are rarely isolated objects and their gravitational…
Connecting the dots: a correlation between ionising radiation and cloud mass-loss rate traced by optical integral field spectroscopy
A. F. McLeod, M. Gritschneder, J. E. Dale +7
We present an analysis of the effect of feedback from O- and B-type stars with data from the integral field spectrograph MUSE mounted on the Very Large Telescope of pillar-like str…
On the IMF in a Triggered Star Formation Context
Tingtao Zhou, Chelsea X. Huang, D. N. C. Lin +2
The origin of the stellar initial mass function (IMF) is a fundamental issue in the theory of star formation. It is generally fit with a composite power law. Some clues on the prog…