Circumplanetary disc properties obtained from radiation hydrodynamical simulations of gas accretion by protoplanets
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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 find ξ ~0.3.
“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
Estimates of the size ratio ξ for circumplanetary disks range from about 0.1 to about 0.4.
“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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An ALMA and MagAO Study of the Substellar Companion GQ Lup B ∗
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ACCRETION OF SOLID MATERIALS ONTO CIRCUMPLANETARY DISKS FROM PROTOPLANETARY DISKS
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Hydrogen Recombination Line Luminosities and Variability from Forming Planets
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PHOTOEVAPORATION AS A TRUNCATION MECHANISM FOR CIRCUMPLANETARY DISKS
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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).”
BackgroundInfluentialAN ALMA CONSTRAINT ON THE GSC 6214-210 B CIRCUM-SUBSTELLAR ACCRETION DISK MASS
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Planet migration, resonant locking, and accretion streams in PDS 70: comparing models and data
Toci, C., Lodato, G., Christiaens, V., Fedele, D., Pinte, C., Price, D. J., & Testi, L. (2020) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/staa2933 · Cited by 34 · see citing works
Gas squeezing during the merger of a supermassive black hole binary
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DISK-FED GIANT PLANET FORMATION
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- 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 › Physics and Astronomy › Astronomy and Astrophysics › 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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