Image Details

Choose export citation format:

Dynamical Formation of the GW190814 Merger

  • Authors: Manuel Arca Sedda

2021 The Astrophysical Journal Letters 908 L38.

  • Provider: AAS Journals

Caption: Figure 6.

Left panel: final mass for compact objects as a function of the ZAMS mass adopted in this work (straight thin red line) in comparison with Ze20 (dashed thick black line), SM17 (dashed thick light-green line), and Be02 (dashed thick light-blue line) models. The light-gray area encompass the supposed lower mass gap, whereas the dark-gray area labels the mass gap featured in our models. Right panel: NS mass spectrum adopted in this work (thick red line) compared with Ze20 (black steps), SM17 (dashed green steps), and Be02 (filled blue steps).

Other Images in This Article
Copyright and Terms & Conditions

Additional terms of reuse