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Tidal torques on accretion discs in binary systems with extreme mass ratios
Abstract
This paper investigates the tidal transport of angular momentum in accretion disc flow in a close binary system with small mass ratio, q. We demonstrate that the disc can only be tidally truncated if q is greater than the inverse of the Reynolds number. We derive the existence of a strong 2:1 resonance. Near the resonance, a spiral dissipation pattern is expected. If the Reynolds number is greater than ∼q−2, a dissipation and angular momentum loss from the disc may be sufficient to truncate it at the resonance. Finally we discuss the application of these results to dwarf novae.
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Cited by
Orbital migration of the planetary companion of 51 Pegasi to its present location
Lin, D. N. C., Bodenheimer, P., & Richardson, D. C. (1996) · Nature · doi:10.1038/380606a0 · Cited by 1,235
Self-citationPlanet-Disk Interaction and Orbital Evolution
Kley, W., & Nelson, R. P. (2012) · Annual Review of Astronomy and Astrophysics · doi:10.1146/annurev-astro-081811-125523 · Cited by 722
Tidal Dissipation in Rotating Giant Planets
Ogilvie, G. I., & Lin, D. N. C. (2004) · The Astrophysical Journal · doi:10.1086/421454 · Cited by 386
Self-citationEscala, A., Larson, R. B., Coppi, P. S., & Mardones, D. (2005) · The Astrophysical Journal · doi:10.1086/431747 · Cited by 317
Formation of the Galilean Satellites in a Gaseous Nebula
Lunine, J. I., & Stevenson, D. J. (1982) · Icarus · doi:10.1016/0019-1035(82)90166-x · Cited by 245
Metadata
- Authors
- Lin, D. N. C., & Papaloizou, J.
- Venue
- Monthly Notices of the Royal Astronomical Society
- Publisher
- Oxford University Press (OUP)
- Published
- 1979-04-01
- Volume
- 186
- Issue
- 4
- Pages
- 799-812
- ISSN
- 0035-8711 (ISSN-L)
- 1365-2966
- OpenAlex
- W2063349913
- Cited by
- 525
- References
- 0
- FWCI
- 8.30
- Type
- journal article
- Language
- en
- Open access
- closed
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- Lin, D. N. C., & Papaloizou, J. (1979). Tidal torques on accretion discs in binary systems with extreme mass ratios. Monthly Notices of the Royal Astronomical Society. https://doi.org/10.1093/mnras/186.4.799
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