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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“The disk aspect ratio of a circumplanetary disk can be significantly larger than that of a circumstellar disk with typical values in the range 0.1–0.3 (Ayliffe & Bate 2009b; Martin & Lubow 2011).”
BackgroundInfluentialGas dynamics around a Jupiter-mass planet
Lega, E., Benisty, M., Cridland, A. J., Morbidelli, A., Schulik, M., & Lambrechts, M. (2024) · Astronomy and Astrophysics · doi:10.1051/0004-6361/202450899 · Cited by 14
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“E-mail: sarah.keith3@students.mq.edu.au; mark.wardle@mq.edu.au the collapse and detachment of the protoplanet envelope from the nebula (Lunine & Stevenson 1982; Ayliffe & Bate 2009a).”
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BackgroundIzquierdo, A. F., Bae, J., Galloway-Sprietsma, M., van Dishoeck, E. F., Facchini, S., Rosotti, G. P., Stadler, J., Benisty, M., & Testi, L. (2026) · The Astrophysical Journal Letters · doi:10.3847/2041-8213/ae2f59 · Cited by 7
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Millimeter Dust Emission and Planetary Dynamics in the HD 106906 System
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“A possible circumplanetary disk must lie within the Hill radius and likely lies within one third of it (Quillen & Trilling 1998; Ayliffe & Bate 2009; Martin & Lubow 2011; Shabram & Boley 2013), so we used both as estimates for the circumplanetary disks radius.”
MethodTaylor, A. G., & Adams, F. C. (2024) · Icarus · doi:10.1016/j.icarus.2024.116327 · Cited by 7
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“Because some material that enters this surface is expected to subsequently leave the Hill sphere (e.g., Ayliffe & Bate 2009; Lambrechts & Lega 2017; Szulágyi et al. 2016), ̇𝑀 is defined here to be the net mass accretion rate onto the planet.”
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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