The DOI matches its Crossref record.
Galactic Dynamics: Second Edition
Overview
Integrity signals
Registry
Cites
Statistics
Verification
Claims the paper makes
Claims other papers make about this one
Each is checked against this paper’s own text: does it say what the citing paper says it does?
In the citing paper
“The CMZ is thought to originate as a result of the gas dynamics within the Galactic bar.”
From The Fermi/eROSITA bubbles: a look into the nuclear outflow from the Milky Way (2024) · cites this paper as Binney & Tremaine 2008
In the citing paper
“Stable orbits in the bar potential ( x 1 orbits) become intersecting when the orbital energy reaches a critical value (Binney & Tremaine 2008).”
From The Fermi/eROSITA bubbles: a look into the nuclear outflow from the Milky Way (2024) · cites this paper as Binney & Tremaine 2008
Citations
Cited by
Sorted by citations
Coevolution (Or Not) of Supermassive Black Holes and Host Galaxies
Kormendy, J., & Ho, L. C. (2013) · Annual Review of Astronomy and Astrophysics · doi:10.1146/annurev-astro-082708-101811 · Cited by 4,421
Harko, T., Lobo, F. S. N., Nojiri, S., & Odintsov, S. D. (2011) · Physical review. D. Particles, fields, gravitation, and cosmology/Physical review. D. Particles and fields · doi:10.1103/physrevd.84.024020 · Cited by 2,888
Local kinematics and the local standard of rest
Schönrich, R. A., Binney, J. J., & Dehnen, W. (2010) · Monthly Notices of the Royal Astronomical Society · doi:10.1111/j.1365-2966.2010.16253.x · Cited by 1,934
“The theoretical underpinning of this method is the asymmetric drift relation (see Binney & Tremaine 2008, eq.”
MethodSelf-citationUltralight scalars as cosmological dark matter
Hui, L., Ostriker, J. P., Tremaine, S. D., & Witten, E. (2017) · Physical review. D/Physical review. D. · doi:10.1103/physrevd.95.043541 · Cited by 1,882
Self-citationgalpy: A python LIBRARY FOR GALACTIC DYNAMICS
Bovy, J. (2015) · The Astrophysical Journal Supplement Series · doi:10.1088/0067-0049/216/2/29 · Cited by 1,655
“…list thereof to be used. solar radius5 R0 for populations with different radial-velocity dispersions and investigate how they depend on the asymmetric drift, i.e., the offset between the mean rotational velocity of a kinematically warm population and the circular velocity (Binney & Tremaine 2008).”
BackgroundMethodResultInfluential
Metadata
- Authors
- Binney, J., & Tremaine, S.
- Venue
- Princeton University Press eBooks
- Publisher
- Princeton University Press
- Published
- 2008-12-31
- OpenAlex
- W1631788275
- Cited by
- 4,375
- References
- 0
- Citations by year
- 2026: 192 · 2025: 224 · 2024: 246 · 2023: 261 · 2022: 233 · 2021: 298 · 2020: 349 · 2019: 372 · 2018: 313 · 2017: 201 · 2016: 252 · 2015: 233 · 2014: 240 · 2013: 233 · 2012: 202
- FWCI
- 138.34
- Type
- book
- Language
- en
- Open access
- closed
- Locations
- Princeton University Press eBooks (publishedVersion)
- Topics
- Physical Sciences › Physics and Astronomy › Astronomy and Astrophysics › Galaxies: Formation, Evolution, Phenomena
- Physical Sciences › Physics and Astronomy › Astronomy and Astrophysics › Stellar, planetary, and galactic studies
- Physical Sciences › Physics and Astronomy › Astronomy and Astrophysics › Astrophysical Phenomena and Observations
- Keywords
- galaxy dynamics, galaxies, stellar dynamics, galaxy structure, galaxy evolution
About these checks
Registry, retraction, Cites and statistics results are computed, not judged, with one exception: a printed reference that no index lists is read once by a model before it counts as a citation error. Claims are extracted by a model and kept only when their quote appears verbatim in the text; each cited source is then checked, with a model’s help, for whether it says what the claim relies on. Those verdicts can be wrong — read the claim’s quote and the cited source before relying on one.
Statistics and arithmetic are recomputed, not judged.
Confidence bands are shown only for fields calibrated on our annotated test set. None is calibrated yet, so no band is shown.
What counts as a claim ›How we measure confidence ›How we check this ›
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