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Potential softening and eccentricity dynamics in razor-thin, nearly-Keplerian discs
In many astrophysical problems involving discs (gaseous or particulate) orbiting a dominant central mass, gravitational potential of the disc plays an important dynamical role. Its impact on the motion of external objects, as well as on the dynamics of the disc itself, can usually be studied using s...
| Autores principales: | , |
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| Formato: | Online Artículo Texto |
| Lenguaje: | English |
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Oxford University Press
2019
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| Acceso en línea: | https://www.ncbi.nlm.nih.gov/pmc/articles/PMC7734392/ https://www.ncbi.nlm.nih.gov/pubmed/33384461 http://dx.doi.org/10.1093/mnras/stz2412 |