The DOI matches its Crossref record; 40 of the 41 references it cites were found in a registry or an index.
Circumplanetary disc properties obtained from radiation hydrodynamical simulations of gas accretion by protoplanets
Open accessAbstract
We investigate the properties of circumplanetary discs formed in three-dimensional, self-gravitating radiation hydrodynamical models of gas accretion by protoplanets. We determine disc sizes, scaleheights, and density and temperature profiles for different protoplanet masses, in solar nebulae of differing grain opacities. We find that the analytical prediction of circumplanetary disc radii in an evacuated gap (RHill/3) from Quillen & Trilling yields a good estimate for discs formed by high-mass protoplanets. The radial density profiles of the circumplanetary discs may be described by power laws between r−2 and r−3/2. We find no evidence for the ring-like density enhancements that have been found in some previous models of circumplanetary discs. Temperature profiles follow a ∼r−7/10 power law regardless of protoplanet mass or nebula grain opacity. The discs invariably have large scaleheights (H/r > 0.2), making them thick in comparison with their encompassing circumstellar discs, and they show no flaring.
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“Martin & Lubow (2011) suggest a tidal truncation limit of ξ ∼ 0 . 4 and hydrodynamic simulations of planets in circumstellar disks find ξ ∼ 0 . 3 (Quillen & Trilling 1998; Ayliffe & Bate 2009).”
From Mass and period limits on the ringed companion transiting the young star J1407 (2015) · cites this paper as Ayliffe & Bate 2009
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“Based on a centripetal radius argument, Quillen & Trilling (1998) estimated that an accreting circumplanetary disk would have ξ = 1/3.Hydrodynamic simulations of planets embedded in circumstellar disks also can find ξ ∼ 0.3 (Ayliffe & Bate 2009).A tidal truncation argument suggests ξ ∼ 0.4 (Martin & Lubow 2011).Theoretical models for Jupiter's circumplanetary disk accounting for Galilean satellite”
From PLANETARY CONSTRUCTION ZONES IN OCCULTATION: DISCOVERY OF AN EXTRASOLAR RING SYSTEM TRANSITING A YOUNG SUN-LIKE STAR AND FUTURE PROSPECTS FOR DETECTING ECLIPSES BY CIRCUMSECONDARY AND CIRCUMPLANETARY DISKS (2012) · cites this paper as Ayliffe & Bate 2009
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Cited by
Sorted by citations
Kinematic Evidence for an Embedded Protoplanet in a Circumstellar Disk
Pinte, C., Price, D. J., Ménard, F., Duchêne, G., Dent, W. R. F., Hill, T., de Gregorio-Monsalvo, I., Hales, A., & Mentiplay, D. (2018) · The Astrophysical Journal Letters · doi:10.3847/2041-8213/aac6dc · Cited by 337
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“Simulations presented by Ayliffe & Bate (2009) suggest that 5 Note that our parametrization is different from the publicly available version of FARGO. the circumplanetary disk has a radius Rcp ≃ RH/3 and aspect ratio (H/R)cp ≃ 0.5.”
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“The above value of rtrunc is in agreement with the point of turnover of specific angular momentum found in their two-dimensional SPH simulation, as well as in the result of Ayliffe & Bate (2009b).”
BackgroundResultInfluential
Metadata
- Authors
- Ayliffe, B. A., & Bate, M. R.
- Affiliations
- University of Exeter (GB)
- Corresponding author
- Ayliffe, Ben A.
- Bate, Matthew R.
- Venue
- Monthly Notices of the Royal Astronomical Society
- Publisher
- Oxford University Press (OUP)
- Published
- 2009-08-01
- Volume
- 397
- Issue
- 2
- Pages
- 657-665
- ISSN
- 0035-8711 (ISSN-L)
- 1365-2966
- OpenAlex
- W2097133096
- Cited by
- 167
- References
- 41
- Citations by year
- 2026: 8 · 2025: 12 · 2024: 11 · 2023: 9 · 2022: 11 · 2021: 11 · 2020: 10 · 2019: 19 · 2018: 10 · 2017: 6 · 2016: 8 · 2015: 10 · 2014: 12 · 2013: 6 · 2012: 10
- FWCI
- 4.03
- Type
- journal article
- Language
- en
- Open access
- bronze
- doi.org
- Locations
- Monthly Notices of the Royal Astronomical Society (publishedVersion)
- arXiv (Cornell University) (submittedVersion)
- arXiv (Cornell University)
- Funders
- Leverhulme Trust
- European Science Foundation
- Science and Technology Facilities Council (PP/D508220/1)
- Topics
- Physical Sciences › Physics and Astronomy › Astronomy and Astrophysics › Astrophysics and Star Formation Studies
- 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
- Keywords
- circumplanetary discs, protoplanets, gas accretion, radiation hydrodynamics, self-gravitating disks, temperature profiles, grain opacity, solar nebula
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