The DOI matches its Crossref record; 1 of the 1 references it cites were found in a registry or an index.
Timescales for planetary accretion and the structure of the protoplanetary disk
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Citations
Cites
Planetesimals to planets: Numerical simulation of collisional evolution
Greenberg, R., Wacker, J. F., Hartmann, W. K., & Chapman, C. R. (1978) · Icarus · doi:10.1016/0019-1035(78)90057-x · Cited by 476
Cited by
The Galactic Center massive black hole and nuclear star cluster
Genzel, R., Eisenhauer, F., & Gillessen, S. (2010) · Reviews of Modern Physics · doi:10.1103/revmodphys.82.3121 · Cited by 1,236
Giant Planet Formation by Gravitational Instability
Boss, A. P. (1997) · Science · doi:10.1126/science.276.5320.1836 · Cited by 1,124
The Two Young Star Disks in the Central Parsec of the Galaxy: Properties, Dynamics, and Formation
Paumard, T., Genzel, R., Martins, F., Nayakshin, S., Beloborodov, A. M., Levin, Y., Trippe, S., Eisenhauer, F., Ott, T., Gillessen, S., et al. (2006) · The Astrophysical Journal · doi:10.1086/503273 · Cited by 690
Gravitational scattering as a possible origin for giant planets at small stellar distances
Weidenschilling, S. J., & Marzari, F. (1996) · Nature · doi:10.1038/384619a0 · Cited by 553
Calculations of the accretion and evolution of giant planets: The effects of solid cores
Bodenheimer, P., & Pollack, J. B. (1986) · Icarus · doi:10.1016/0019-1035(86)90122-3 · Cited by 512
Metadata
- Authors
- Lissauer, J. J.
- Venue
- Icarus
- Publisher
- Elsevier BV
- Published
- 1987-02
- Volume
- 69
- Issue
- 2
- Pages
- 249-265
- ISSN
- 0019-1035 (ISSN-L)
- OpenAlex
- W2004651075
- Cited by
- 480
- References
- 1
- FWCI
- 9.32
- Type
- journal article
- Language
- en
- Open access
- closed
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.
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How to cite
Cite CoChat for the checks on this page, and the paper for its own findings.
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- CoChat. (2026). Citation check: Timescales for planetary accretion and the structure of the protoplanetary disk. https://app.cochat.ai/papers/10.1016/0019-1035(87)90104-7
- The paper
- Lissauer, J. J. (1987). Timescales for planetary accretion and the structure of the protoplanetary disk. Icarus. https://doi.org/10.1016/0019-1035(87)90104-7
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.
