Cited by 665Galaxies: Formation, Evolution, PhenomenaCosmology and Gravitation TheoriesStellar, planetary, and galactic studies

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Radial Acceleration Relation in Rotationally Supported Galaxies

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McGaugh, Stacy S., Lelli, Federico, Schombert, James M.·2016·Physical Review Letters

DOI 10.1103/physrevlett.117.201101

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Abstract

We report a correlation between the radial acceleration traced by rotation curves and that predicted by the observed distribution of baryons. The same relation is followed by 2693 points in 153 galaxies with very different morphologies, masses, sizes, and gas fractions. The correlation persists even when dark matter dominates. Consequently, the dark matter contribution is fully specified by that of the baryons. The observed scatter is small and largely dominated by observational uncertainties. This radial acceleration relation is tantamount to a natural law for rotating galaxies.

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Authors: McGaugh, S. S., Lelli, F., & Schombert, J. M.
Affiliations: Case Western Reserve University (US)
University of Oregon (US)
ORCID: McGaugh, Stacy S.
Lelli, Federico
Schombert, James M.
Venue: Physical Review Letters
Publisher: American Physical Society (APS)
Published: 2016-11-09
Volume: 117
Issue: 20
Pages: 201101-201101
ISSN: 0031-9007 (ISSN-L)
1079-7114
DOI: 10.1103/physrevlett.117.201101
OpenAlex: W2523266658
Cited by: 665
References: 53
Citations by year: 2026: 71 · 2025: 49 · 2024: 53 · 2023: 66 · 2022: 69 · 2021: 67 · 2020: 78 · 2019: 69 · 2018: 64 · 2017: 67 · 2016: 12
FWCI: 33.79
Type: journal article
Language: en
Open access: green
arxiv.org
Licence: link.aps.org/licenses/aps-default-license (vor)
link.aps.org/licenses/aps-default-accepted-manuscript-license (am, 365 d)
Locations: Physical Review Letters (publishedVersion)
PubMed (publishedVersion)
arXiv (Cornell University) (submittedVersion)
Scholarly Commons @ Case Western Reserve University (submittedVersion)
arXiv (Cornell University)
Funders: Jet Propulsion Laboratory
California Institute of Technology
National Aeronautics and Space Administration (NNX13AH32G)
John Templeton Foundation
Topics: Physical Sciences › Physics and Astronomy › Astronomy and Astrophysics › Galaxies: Formation, Evolution, Phenomena
Physical Sciences › Physics and Astronomy › Astronomy and Astrophysics › Cosmology and Gravitation Theories
Physical Sciences › Physics and Astronomy › Astronomy and Astrophysics › Stellar, planetary, and galactic studies
Keywords: radial acceleration relation, rotation curves, baryonic Tully-Fisher relation, dark matter, baryon distribution, galaxy morphology, galaxy mass, void fraction

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Radial Acceleration Relation in Rotationally Supported Galaxies

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