Supplementary movies for "A unified model for the co-evolution of galaxies and their circumgalactic medium: the relative roles of turbulence and atomic cooling physics"
=== Title: A unified model for the co-evolution of galaxies and their circumgalactic medium: the relative roles of turbulence and atomic cooling physics Authors: Pandya V., Fielding D.B., Bryan G.L., Carr C., Somerville R.S., Stern J., Faucher-Giguere C.-L., Hafen Z., Angles-Alcazar D., Forbes J.C....
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Title: A unified model for the co-evolution of galaxies and their
circumgalactic medium: the relative roles of turbulence and
atomic cooling physics
Authors: Pandya V., Fielding D.B., Bryan G.L., Carr C., Somerville R.S.,
Stern J., Faucher-Giguere C.-L., Hafen Z., Angles-Alcazar D., Forbes J.C.
===
Description of contents: This Dataverse deposit includes supplementary movies for various simulated dark matter halos as described in the accepted version of the article listed above. The movies show the time evolution of the equilibrium temperature and turbulent velocity for the circumgalactic medium based on a novel semi-analytic model.
A list of the individual files and halos are given
below.
Halo Animation Description
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m10q supplementary_animation_m10q.mp4 ultrafaint dwarf, Mvir~10+10Msun
m10y supplementary_animation_m10y.mp4 ultrafaint dwarf, Mvir~10+10Msun
m10z supplementary_animation_m10z.mp4 ultrafaint dwarf, Mvir~10+10Msun
m11a supplementary_animation_m11a.mp4 intermediate-mass dwarf, Mvir~10+11 Msun
m11c supplementary_animation_m11c.mp4 intermediate-mass dwarf, Mvir~10+11 Msun
m11b supplementary_animation_m11b.mp4 intermediate-mass dwarf, Mvir~10+11 Msun
m11f supplementary_animation_m11f.mp4 intermediate-mass dwarf, Mvir~10+11 Msun
m11q supplementary_animation_m11q.mp4 intermediate-mass dwarf, Mvir~10+11 Msun
m11v supplementary_animation_m11v.mp4 intermediate-mass dwarf, Mvir~10+11 Msun
m12f supplementary_animation_m12f.mp4 MW-mass halo, Mvir~10+12 Msun
m12i supplementary_animation_m12i.mp4 MW-mass halo, Mvir~10+12 Msun
m12m supplementary_animation_m12m.mp4 MW-mass halo, Mvir~10+12 Msun; also shown in the accepted article as Figure 14)
System requirements: These are all standard H.264 encoded, MP4 animations.
Additional comments: The movies were created based on a semi-analytic model that treats the co-evolution of galaxies and their circumgalactic medium. The panels and main takeaways of the movies are described in the caption of Figure 14 from the article referenced above.
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DOI: | 10.7910/dvn/ki1b0e |