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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

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.

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 Creators:
van Son, L. A. C.1, Author           
de Mink, S. E.2, Author           
Chruslinska, Martyna2, Author           
Conroy, C., Author
Pakmor, R.2, Author           
Hernquist, L., Author
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1MPI for Astrophysics, Max Planck Society, ou_159875              
2Stellar Astrophysics, MPI for Astrophysics, Max Planck Society, ou_159882              

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 Dates: 2023-05-11
 Publication Status: Published online
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 Identifiers: DOI: 10.3847/1538-4357/acbf51
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Title: The Astrophysical Journal
Source Genre: Journal
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Publ. Info: Bristol; Vienna : IOP Publishing; IAEA
Pages: - Volume / Issue: 948 (2) Sequence Number: 105 Start / End Page: - Identifier: ISSN: 0004-637X
CoNE: https://pure.mpg.de/cone/journals/resource/954922828215_3