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Cited by 382

The DOI matches its Crossref record; 1 of the 1 references it cites were found in a registry or an index.

Consequences of Gravitational Radiation Recoil

Open access
Merritt, David, Milosavljevi, Milo, Favata, Marc, Hughes, Scott A., Holz, Daniel E.·2004·The Astrophysical Journal

Abstract

Coalescing binary black holes experience an impulsive kick from anisotropic emission of gravitational waves. Recoil velocities are sufficient to eject most coalescing black holes from dwarf galaxies and globular clusters, which may explain the apparent absence of massive black holes in these systems. Ejection from giant elliptical galaxies would be rare, but coalescing black holes are displaced from the center and fall back on a timescale of order the half-mass crossing time. Displacement of the black holes transfers energy to the stars in the nucleus and can convert a steep density cusp into a core. Radiation recoil calls into question models that grow supermassive black holes from hierarchical mergers of stellar-mass precursors.

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Crossref · 10.1086/421551

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Metadata

Authors
Merritt, D., Milosavljevi, M., Favata, M., Hughes, S. A., & Holz, D. E.
Venue
The Astrophysical Journal
Published
2004-04-20
Volume
607
Issue
1
Pages
L9-L12
ISSN
  • 0004-637X (ISSN-L)
  • 1538-4357
OpenAlex
W2097690225
Cited by
382
References
1
FWCI
15.75
Type
journal article
Language
en
Open access
bronze

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CoChat. (2026). Citation check: Consequences of Gravitational Radiation Recoil. https://app.cochat.ai/papers/10.1086/421551
The paper
Merritt, D., Milosavljevi, M., Favata, M., Hughes, S. A., & Holz, D. E. (2004). Consequences of Gravitational Radiation Recoil. The Astrophysical Journal. https://doi.org/10.1086/421551

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Bibliographic data: Semantic Scholar, OpenAlex, Crossref.

Contains information from the Semantic Scholar Academic Graph Datasets, made available under the ODC Attribution License (ODC-BY 1.0).

Semantic Scholar’s data is described in: Kinney, R., et al. (2023). The Semantic Scholar Open Data Platform. arXiv:2301.10140.