English
 
Help Privacy Policy Disclaimer
  Advanced SearchBrowse

Item

ITEM ACTIONSEXPORT
Add to Basket
  Local TagsRelease HistoryDetailsSummary

Released
Journal Article

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

MPS-Authors
/persons/resource/persons271079

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

/persons/resource/persons266173

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

/persons/resource/persons282178

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

/persons/resource/persons4732

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

External Resource
No external resources are shared
Fulltext (restricted access)
There are currently no full texts shared for your IP range.
Fulltext (public)
There are no public fulltexts stored in PuRe
Supplementary Material (public)
There is no public supplementary material available
Citation

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
Abstract
There is no abstract available