The DOI matches its Crossref record.
II. Spiral Arms as Sheared Gravitational Instabilities
Open accessAbstract
This paper treats examples of gravitational instability in differentially rotating media. The particular cases dealt with include polytropic, stratified sheets of gas, as well as the infinite homogeneous media. Application of the results is made to the formation of spiral arms in a differentially rotating disk galaxy. Relations are derived which connect the thickness of the galactic disk, its density, and the velocity dispersion perpendicular to the galactic plane with Oort's differential rotation parameters A and B . Sections 1 and 2 discuss requirements of any theory of spiral arms. Sections 3 to 8 give a mathematical treatment of gravitational instability in a sheared rotating stratified medium. Section 9 discusses these results qualitatively and proposes a theory of spiral arm formation based on them. Section 10 gives the observational tests and consequences of the theory. Finally Section 11 gives a very brief discussion of barred spirals and points to the many problems left unsolved by the present work.
Overview
The claims and statistics of this paper haven’t been checked yet.
Run the check — free, no account needed. It reads the open-access text and checks the sources it cites.
Integrity signals
Registry
Cites
Statistics
Verification
Claims the paper makes
The claims and statistics of this paper haven’t been checked yet.
Run the check — free, no account needed. It reads the open-access text and checks the sources it cites.
Self-check
Percentages, sums and reported differences re-computed from the paper’s own numbers.
The self-check needs the paper’s full text.
Citations
Cited by
Star Formation Thresholds and Galaxy Edges: Why and Where
Schaye, J. (2004) · The Astrophysical Journal · doi:10.1086/421232 · Cited by 615
Rapid Formation of Molecular Clouds and Stars in the Solar Neighborhood
Hartmann, L., Ballesteros‐Paredes, J., & Bergin, E. A. (2001) · The Astrophysical Journal · doi:10.1086/323863 · Cited by 567
Linear and non-linear evolution of the vertical shear instability in accretion discs
Nelson, R. P., Gressel, O., & Umurhan, O. M. (2013) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/stt1475 · Cited by 444
What controls star formation in the central 500 pc of the Galaxy?
Kruijssen, J. M. D., Longmore, S. N., Elmegreen, B. G., Murray, N., Bally, J., Testi, L., & Kennicutt, R. C. (2014) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/stu494 · Cited by 288
Bland-Hawthorn, J., Sharma, S., Tepper-Garcia, T., Binney, J., Freeman, K. C., Hayden, M. R., Kos, J., De Silva, G. M., Ellis, S., Lewis, G. F., et al. (2019) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/stz217 · Cited by 224
Metadata
- Authors
- Goldreich, P., & Lynden-Bell, D.
- Venue
- Monthly Notices of the Royal Astronomical Society
- Publisher
- Oxford University Press (OUP)
- Published
- 1965-08-01
- Volume
- 130
- Issue
- 2
- Pages
- 125-158
- ISSN
- 0035-8711 (ISSN-L)
- 1365-2966
- OpenAlex
- W1985873501
- Cited by
- 945
- References
- 0
- FWCI
- 2.17
- Type
- journal article
- Language
- en
- Open access
- bronze
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 ›
Are you an author, or do you see a problem with this page? Request a review
How to cite
Cite CoChat for the checks on this page, and the paper for its own findings.
- This page
- CoChat. (2026). Citation check: II. Spiral Arms as Sheared Gravitational Instabilities. https://app.cochat.ai/papers/10.1093/mnras/130.2.125
- The paper
- Goldreich, P., & Lynden-Bell, D. (1965). II. Spiral Arms as Sheared Gravitational Instabilities. Monthly Notices of the Royal Astronomical Society. https://doi.org/10.1093/mnras/130.2.125
Data sources
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.