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Delayed and Displaced: The Impact of Binary Interactions on Core-collapse SN Feedback

  • Authors: Tom Wagg, Julianne J. Dalcanton, Mathieu Renzo, Katelyn Breivik, Matthew E. Orr, Adrian M. Price-Whelan, Akaxia Cruz, Alyson Brooks, Ulrich P. Steinwandel, Eric C. Bellm

Tom Wagg et al 2025 The Astronomical Journal 170 .

  • Provider: AAS Journals

Caption: Figure 14.

The total number of SNe that occur for each variation, separated by progenitor type (variations are outlined in Section 4.1). Dotted lines and shaded regions show the fiducial value and a ±15% region around this value. The exact values for each variation are given in Table C1. The solid black line shows the total for a population of single stars that is equivalent to our fiducial model, indicating that binary models typically increase the total SN feedback in a population. The line does not continue for all variations, since the later ones would alter a single star population as well. An interactive version of this data is available in Figure 12.

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