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Dynamical friction in spherical systems
Open accessAbstract
We investigate dynamical friction on a test object (such as a bar or satellite) which rotates or revolves through a spherical stellar system. We find that frictional effects arise entirely from near-resonant stars and we derive an analog to Chandrasekhar's dynamical friction formula which applies to spherical systems. We show that a formula of this type is valid so long as the angular speed of the test object changes sufficiently rapidly. If the angular speed is slowly changing two new effects appear: a reversible dynamical feedback which can stabilize or destabilize the rotation speed, and permanent capture of near-resonant stars into librating orbits. We discuss orbital decay of satellites in the light of these results.
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Cited by
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Ward, W. R. (1997) · Icarus · doi:10.1006/icar.1996.5647 · Cited by 1,071
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Constraints from Dynamical Friction on the Dark Matter Content of Barred Galaxies
Debattista, V. P., & Sellwood, J. A. (2000) · The Astrophysical Journal · doi:10.1086/317148 · Cited by 560
Bar-Halo Interaction and Bar Growth
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Metadata
- Authors
- Tremaine, S., & Weinberg, M. D.
- Venue
- Monthly Notices of the Royal Astronomical Society
- Publisher
- Oxford University Press (OUP)
- Published
- 1984-08-01
- Volume
- 209
- Issue
- 4
- Pages
- 729-757
- ISSN
- 0035-8711 (ISSN-L)
- 1365-2966
- OpenAlex
- W2052986856
- Cited by
- 313
- References
- 0
- FWCI
- 2.61
- Type
- journal article
- Language
- en
- Open access
- bronze
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- Tremaine, S., & Weinberg, M. D. (1984). Dynamical friction in spherical systems. Monthly Notices of the Royal Astronomical Society. https://doi.org/10.1093/mnras/209.4.729
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