The Kozai-Lidov mechanism in hydrodynamical disks
dc.contributor.author | Martin R.G. | |
dc.contributor.author | Nixon C. | |
dc.contributor.author | Lubow S.H. | |
dc.contributor.author | Armitage P.J. | |
dc.contributor.author | Price D.J. | |
dc.contributor.author | Dogan S. | |
dc.contributor.author | King A. | |
dc.date.accessioned | 2019-10-26T21:27:34Z | |
dc.date.available | 2019-10-26T21:27:34Z | |
dc.date.issued | 2014 | |
dc.department | Ege Üniversitesi | en_US |
dc.description.abstract | We use three-dimensional hydrodynamical simulations to show that a highly misaligned accretion disk around one component of a binary system can exhibit global Kozai-Lidov cycles, where the inclination and eccentricity of the disk are interchanged periodically. This has important implications for accreting systems on all scales, for example, the formation of planets and satellites in circumstellar and circumplanetary disks, outbursts in X-ray binary systems, and accretion onto supermassive black holes. © 2014. The American Astronomical Society. All rights reserved.. | en_US |
dc.description.sponsorship | National Aeronautics and Space Administration, NASA National Aeronautics and Space Administration, NASA: NNX11AK61G | en_US |
dc.identifier.doi | 10.1088/2041-8205/792/2/L33 | |
dc.identifier.issn | 2041-8205 | |
dc.identifier.issn | 2041-8205 | en_US |
dc.identifier.issue | 2 | en_US |
dc.identifier.scopusquality | Q1 | en_US |
dc.identifier.uri | https://doi.org/10.1088/2041-8205/792/2/L33 | |
dc.identifier.uri | https://hdl.handle.net/11454/17421 | |
dc.identifier.volume | 792 | en_US |
dc.indekslendigikaynak | Scopus | en_US |
dc.language.iso | en | en_US |
dc.publisher | Institute of Physics Publishing | en_US |
dc.relation.ispartof | Astrophysical Journal Letters | en_US |
dc.relation.publicationcategory | Makale - Uluslararası Hakemli Dergi - Kurum Öğretim Elemanı | en_US |
dc.rights | info:eu-repo/semantics/openAccess | en_US |
dc.subject | accretion accretion disks | en_US |
dc.subject | binaries: general | en_US |
dc.subject | black hole physics | en_US |
dc.subject | hydrodynamics | en_US |
dc.subject | planets and satellites: formation | en_US |
dc.subject | stars: emission-line Be | en_US |
dc.title | The Kozai-Lidov mechanism in hydrodynamical disks | en_US |
dc.type | Article | en_US |