The DOI matches its Crossref record.
Tidal friction in early-type stars
Abstract
Theoretical and observational results related to tides in early-type stars are summarized. The results suggest that the tidal torque on an early-type star is concentrated near the boundary between the convective core and the radiative envelope, and that a train of gravity waves which is excited at this boundary outwardly transports the angular momentum removed from the fluid by the torque. Tidal despinning to synchronous rotation is shown to proceed from the outside to the inside of the star. The present model can account for the previous finding that Zahn's (1975, 1977) theory for tidal evolution in early-type close binaries is compatible with the observed rates of orbit circularization, while significantly underestimating the observed rates of spin synchronization.
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
Accurate masses and radii of normal stars
Andersen, J. (1991) · The Astronomy and Astrophysics Review · doi:10.1007/bf00873538 · Cited by 675
On the Tidal Inflation of Short‐Period Extrasolar Planets
Bodenheimer, P., Lin, D. N. C., & Mardling, R. A. (2001) · The Astrophysical Journal · doi:10.1086/318667 · Cited by 415
Tidal Dissipation in Rotating Giant Planets
Ogilvie, G. I., & Lin, D. N. C. (2004) · The Astrophysical Journal · doi:10.1086/421454 · Cited by 386
Perryman, M. (2018) · Cambridge University Press eBooks · doi:10.1017/9781108304160 · Cited by 340
THERMAL TIDES IN FLUID EXTRASOLAR PLANETS
Arras, P., & Socrates, A. (2010) · The Astrophysical Journal · doi:10.1088/0004-637x/714/1/1 · Cited by 147
Metadata
- Authors
- Goldreich, P., & Nicholson, P. D.
- Venue
- The Astrophysical Journal
- Publisher
- American Astronomical Society
- Published
- 1989-07
- Volume
- 342
- Pages
- 1079
- ISSN
- 0004-637X (ISSN-L)
- 1538-4357
- OpenAlex
- W2022561937
- Cited by
- 229
- References
- 0
- FWCI
- 2.06
- 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.
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: Tidal friction in early-type stars. https://app.cochat.ai/papers/10.1086/167665
- The paper
- Goldreich, P., & Nicholson, P. D. (1989). Tidal friction in early-type stars. The Astrophysical Journal. https://doi.org/10.1086/167665
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.