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The locations of features in the mass distribution of merging binary black holes are robust against uncertainties in the metallicity-dependent cosmic star formation history

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van Son,  L. A. C.
MPI for Astrophysics, Max Planck Society;

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de Mink,  S. E.
Stellar Astrophysics, MPI for Astrophysics, Max Planck Society;

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Chruslinska,  Martyna
Stellar Astrophysics, MPI for Astrophysics, Max Planck Society;

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Pakmor,  R.
Stellar Astrophysics, MPI for Astrophysics, Max Planck Society;

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van Son, L. A. C., de Mink, S. E., Chruslinska, M., Conroy, C., Pakmor, R., & Hernquist, L. (2023). The locations of features in the mass distribution of merging binary black holes are robust against uncertainties in the metallicity-dependent cosmic star formation history. The Astrophysical Journal, 948(2): 105. doi:10.3847/1538-4357/acbf51.


Cite as: https://hdl.handle.net/21.11116/0000-000D-A395-2
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