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Cosmological simulations of the high-redshift galaxy population adopting a variable stellar initial mass function
Anna Durrant, Robert A. Crain, Cedric G. Lacey +15
JWST surveys reveal a greater space density of high-redshift UV-bright galaxies than predicted by conventional galaxy formation models. We present results from a cMpc cosmo…
Variation of the low-mass end of the stellar initial mass function with redshift and metallicity
Matthew R. Bate
We report the stellar mass functions obtained from 20 radiation hydrodynamical simulations of star cluster formation in 500 M molecular clouds with metallicities of 3, 1, 1…
The formation of clusters and OB associations in different density spiral arm environments
C. L. Dobbs, T. J. R. Bending, A. R. Pettitt +2
We present simulations of the formation and evolution of clusters in spiral arms. The simulations follow two different spiral arm regions, and the total gas mass is varied to produ…
Dust coagulation during the early stages of star formation: molecular cloud collapse and first hydrostatic core evolution
Matthew R. Bate
Planet formation in protoplanetary discs requires dust grains to coagulate from the sub-micron sizes that are found in the interstellar medium into much larger objects. For the fir…
Supernovae and photoionizing feedback in spiral arm molecular clouds
Thomas J. R. Bending, Clare L. Dobbs, Matthew R. Bate
We explore the interplay between supernovae and the ionizing radiation of their progenitors in star forming regions. The relative contributions of these stellar feedback processes…
The formation of massive stellar clusters in converging galactic flows with photoionisation
C. L. Dobbs, T. J. R. Bending, A. R. Pettitt +1
We have performed simulations of cluster formation along two regions of a spiral arm taken from a global Milky Way simulation, including photoionising feedback. One region is chara…