478 citations · 8.2k across the 106 of their papers we have counts for
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Non-Equilibrium Abundances Treated Holistically (NEATH): the molecular composition of star-forming clouds
F. D. Priestley, P. C. Clark, S. C. O. Glover +4
Much of what we know about molecular clouds, and by extension star formation, comes from molecular line observations. Interpreting these correctly requires knowledge of the underly…
From dark matter halos to pre-stellar cores: High resolution follow-up of cosmological Lyman-Werner simulations
Lewis R. Prole, Anna T. P. Schauer, Paul C. Clark +3
Molecular hydrogen allows cooling in primordial gas, facilitating its collapse into Population III stars within primordial halos. Lyman-Werner (LW) radiation from these stars can e…
Do simulated molecular clouds look like real ones?
F. D. Priestley, P. C. Clark, A. P Whitworth
Simulations of molecular clouds often begin from highly idealised initial conditions, such as a uniform-density sphere with an artificially imposed turbulent velocity field. While…