The DOI matches its Crossref record; 3 of the 4 references it cites were found in a registry or an index.
How high can a mountain be?
Overview
Integrity signals
Registry
Cites
Statistics
Verification
Claims the paper makes
Citations
Cites
Baym, G., & Pethick, C. (1979) · Annual Review of Astronomy and Astrophysics · doi:10.1146/annurev.aa.17.090179.002215 · Cited by 279
Mechanical engineer's handbook
(2002) · Choice Reviews Online · doi:10.5860/choice.39-3992 · Cited by 174
Mechanical engineers' handbook
Marks, L. S. (2012) · Virtual Defense Library (Ministerio de Defensa) · Cited by 55
Research works printed but not linked: 2
- Elder, J. 1976.The Bowels of the Earth, Oxford University Press.
- Irvine, J. M. 1978,Neutron Stars, Clarendon Press, Oxford.
Cited by
Linear analysis of incompressible Rayleigh-Taylor instability in solids
Piriz, A. R., Cela, J. J. L., & Tahir, N. A. (2009) · Physical Review E · doi:10.1103/physreve.80.046305 · Cited by 77
Elastic-plastic Rayleigh-Taylor instability at a cylindrical interface
Piriz, A. R., Piriz, S. A., & Tahir, N. A. (2021) · Physical review. E · doi:10.1103/physreve.104.035102 · Cited by 18
Gravity defied from potato asteroids to magnetised neutron stars
Konar, S. (2017) · Resonance · doi:10.1007/s12045-017-0455-4 · Cited by 3
Gravitational waves from surface inhomogeneities of neutron stars
Konar, S., Mukherjee, D., Bhattacharya, D., & Sarkar, P. (2016) · Physical review. D/Physical review. D. · doi:10.1103/physrevd.94.104036 · Cited by 3
Gravity defied from potato asteroids to magnetised neutron stars
Konar, S. (2017) · Resonance · doi:10.1007/s12045-017-0490-1
Metadata
- Authors
- Scheuer, P. A. G.
- Affiliations
- University of Cambridge (GB)
- Corresponding author
- Scheuer, P. A. G.
- Venue
- Journal of Astrophysics and Astronomy
- Published
- 1981-06
- Volume
- 2
- Issue
- 2
- Pages
- 165-169
- ISSN
- 0250-6335 (ISSN-L)
- 0973-7758
- OpenAlex
- W2050242245
- Semantic Scholar
- dbd5ca1636de54c37c5bcdc156ac74ba2dd3d865
- Cited by
- 7
- References
- 4
- Citations by year
- 2025: 1 · 2024: 1 · 2021: 1 · 2017: 2 · 2016: 1
- FWCI
- 0.00
- Type
- journal article
- Language
- en
- Open access
- closed
- Licence
- www.springer.com/tdm (tdm)
- Locations
- Journal of Astrophysics and Astronomy (publishedVersion)
- Topics
- Physical Sciences › Earth and Planetary Sciences › Space and Planetary Science › Astro and Planetary Science
- Physical Sciences › Physics and Astronomy › Astronomy and Astrophysics › Stellar, planetary, and galactic studies
- Physical Sciences › Physics and Astronomy › Astronomy and Astrophysics › Pulsars and Gravitational Waves Research
- Keywords
- mountain height, self-gravitating bodies, rock strength, neutron stars
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.
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How to cite
Cite CoChat for the checks on this page, and the paper for its own findings.
- This page
- CoChat. (2026). Citation check: How high can a mountain be? https://app.cochat.ai/papers/10.1007/bf02715676
- The paper
- Scheuer, P. A. G. (1981). How high can a mountain be? Journal of Astrophysics and Astronomy. https://doi.org/10.1007/bf02715676
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.