Orbital migration of the planetary companion of 51 Pegasi to its present location
Integrity signals
Registry
Cites
Statistics
Claims the paper makes
Cited by
Sorted by citations
Atmospheric escape from hot Jupiters
Murray-Clay, R. A., Chiang, E. I., & Murray, N. (2009) · The Astrophysical Journal · doi:10.1088/0004-637x/693/1/23 · Cited by 723 · see citing works
Models of giant planet formation with migration and disc evolution
Alibert, Y., Mordasini, C., Benz, W., & Winisdoerffer, C. (2005) · Astronomy & Astrophysics · doi:10.1051/0004-6361:20042032 · Cited by 685 · see citing works
Dawson, R. I., & Johnson, J. A. (2018) · Annual Review of Astronomy and Astrophysics · doi:10.1146/annurev-astro-081817-051853 · Cited by 622 · see citing works
The interiors of giant planets: Models and outstanding questions.
Guillot, T. (2005) · Annual Review of Earth and Planetary Sciences · doi:10.1146/annurev.earth.32.101802.120325 · Cited by 524 · see citing works
WASP-17b: AN ULTRA-LOW DENSITY PLANET IN A PROBABLE RETROGRADE ORBIT
Anderson, D. R., Hellier, C., Gillon, M., Triaud, A. H. M. J., Smalley, B., Hebb, L., Cameron, A. C., Maxted, P. F. L., Queloz, D., West, R. G., et al. (2010) · The Astrophysical Journal · doi:10.1088/0004-637x/709/1/159 · Cited by 208 · see citing works
- Authors
- Lin, D. N. C., Bodenheimer, P., & Richardson, D. C.
- Affiliations
- University of California, Santa Cruz (US)
- University of Toronto (CA)
- Venue
- Nature
- Published
- 1996-04
- Volume
- 380
- Issue
- 6575
- Pages
- 606-607
- ISSN
- 0028-0836 (ISSN-L)
- 1476-4687
- OpenAlex
- W1967245741
- Cited by
- 1,235
- References
- 0
- Citations by year
- 2026: 37 · 2025: 38 · 2024: 52 · 2023: 37 · 2022: 37 · 2021: 38 · 2020: 40 · 2019: 42 · 2018: 56 · 2017: 52 · 2016: 63 · 2015: 39 · 2014: 52 · 2013: 45 · 2012: 55
- FWCI
- 29.80
- Type
- journal article
- Language
- en
- Open access
- closed
- Licence
- www.springer.com/tdm (tdm)
- Locations
- Nature (publishedVersion)
- University Libraries (University of Maryland) (submittedVersion)
- Topics
- Physical Sciences › Physics and Astronomy › Astronomy and Astrophysics › Stellar, planetary, and galactic studies
- Physical Sciences › Physics and Astronomy › Astronomy and Astrophysics › Astro and Planetary Science
- Physical Sciences › Physics and Astronomy › Astronomy and Astrophysics › Astrophysics and Star Formation Studies
- Keywords
- 51 Pegasi b, exoplanets, planet migration, planet formation, circumstellar disks, gas capture, tidal interactions, stellar magnetospheres, disk truncation, radial velocity variations, gas giant planets
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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