478 citations · 8.2k across the 106 of their papers we have counts for
106 papers
The fragmentation of molecular clouds in starburst environments
Matt T. Cusack, Paul C. Clark, Simon C. O. Glover +4
A significant amount of star formation occurs and has occurred in environments unlike the solar neighbourhood. The majority of stars formed closer to the peak of the cosmic star fo…
Do stars still form in molecular gas within CO-dark dwarf galaxies?
David J. Whitworth, Rowan J. Smith, Simon C. O. Glover +6
In the Milky Way and other main-sequence galaxies, stars form exclusively in molecular gas, which is traced by CO emission. However, low metallicity dwarf galaxies are often `CO-da…
Self-consistent modelling of the Milky Way structure using live potentials
Eva Durán-Camacho, Ana Duarte-Cabral, Alex R. Pettitt +6
To advance our understanding of the evolution of the interstellar medium (ISM) of our Galaxy, numerical models of Milky Way (MW) type galaxies are widely used. However, most models…
Assessing the accuracy of the star formation rate measurements by direct star count in molecular clouds
Sami Dib, Jian Wen Zhou, Sébastien Comerón +8
Star formation estimates based on the counting of YSOs is commonly applied to nearby star-forming regions in the Galaxy. With this method, the SFRs are measured using the counts of…
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…