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The Binary Black Hole Merger Rate Deviates from the Cosmic Star Formation Rate: A Tug of War between Metallicity and Delay Times

  • Authors: Adam P. Boesky, Floor S. Broekgaarden, Edo Berger

Adam P. Boesky et al 2024 The Astrophysical Journal 976 .

  • Provider: AAS Journals

Caption: Figure 11.

The assumed SFRD colored by the stars’ initial metallicity, Z i , for the different MSSFRs from Figure 10. The MSSFR labels are indicated above each panel, and the dotted lines show the redshift location of a few mean metallicities (i.e., the average metallicity of stars formed at a given redshift).

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