A bottleneck for star formation: the importance of magnetic fields during the formation of cold gas in galaxies- solar galaxy projection data

Binary projections files associated with "A bottleneck for star formation: the importance of magnetic fields during the formation of cold gas in galaxies" by McGuinness, Smith, & Whitworth 2025. The data is free to use provided the original publication and source is clearly attributed. Full details of the low metallicity dwarf galaxy simulation used can be found in the above papers. For all queries, contact rjs22 @ st-andrews.ac.ukFiles provided are projection (5kpc diameter centred on the galaxy centre) of thedensity - Column densityxH2 - molecular hydrogen abundance relative to protonsxHP - ionised hydrogen abundance relative to protons, from which HI abundance can be calculated from conservation lawmagnetic_proj - the projected magnetic field strength in each dimension For the original Arepo voronoi grids (and assistance in reading them) please contact the authors.