1.1k citations · 24.6k across the 330 of their papers we have counts for
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Reconstructing three-dimensional densities from two-dimensional observations of molecular gas
Zipeng Hu, Mark R. Krumholz, Christoph Federrath +2
Star formation has long been known to be an inefficient process, in the sense that only a small fraction of the mass of any given gas cloud is converted to stars per c…
Pre-supernova feedback mechanisms drive the destruction of molecular clouds in nearby star-forming disc galaxies
Mélanie Chevance, J. M. Diederik Kruijssen, Mark R. Krumholz +28
It is a major open question which physical processes stop the accretion of gas onto giant molecular clouds (GMCs) and limit the efficiency at which gas is converted into stars with…
The Catalogue for Astrophysical Turbulence Simulations (CATS)
B. Burkhart, S. Appel, S. Bialy +18
Turbulence is a key process in many fields of astrophysics. Advances in numerical simulations of fluids over the last several decades have revolutionized our understanding of turbu…
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…
An uncertainty principle for star formation -- V. The influence of dust extinction on star formation rate tracer lifetimes and the inferred molecular cloud lifecycle
Daniel T. Haydon, Yusuke Fujimoto, Mélanie Chevance +3
Recent observational studies aiming to quantify the molecular cloud lifecycle require the use of known 'reference time-scales' to turn the relative durations of different phases of…
Evolution of Stellar Feedback in HII Regions
Grace M. Olivier, Laura A. Lopez, Anna L. Rosen +4
Stellar feedback is needed to produce realistic giant molecular clouds (GMCs) and galaxies in simulations, but due to limited numerical resolution, feedback must be implemented usi…