Image Details
Caption: Figure 7.
The same as Figure 4, except varying different choices of galaxy settings. SNe timing is unaffected by galaxy settings, but SNe location is strongly dependent on the choice of initial cluster velocity dispersion (though a tail of distant ejected secondary SNe still exists with a low dispersion). An interactive version of this data is available in Figure 4.
© 2025. The Author(s). Published by the American Astronomical Society.