Showing 1 - 20 results of 65 for search '"orbital resonance"', query time: 0.32s Refine Results
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    Exoplanet Predictions Based on Harmonic Orbit Resonances by Markus J. Aschwanden, Felix Scholkmann

    Published 2017-09-01
    “…While earlier studies used a logarithmic spacing, which lacks a physical model, we employ here the theory of harmonic orbit resonances, which contains quantized ratios instead, to explain the observed planet distance ratios and to predict undetected exoplanets. …”
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    Hints of Spin-Orbit Resonances in the Binary Black Hole Population by Varma, Vijay, Biscoveanu, Sylvia, Isi, Maximiliano, Farr, Will M, Vitale, Salvatore

    Published 2022
    “…In particular, the spin orientations of the component black holes within the orbital plane, ϕ_{1} and ϕ_{2}, can be used to identify binaries caught in the so-called spin-orbit resonances. In a companion paper, we demonstrate that ϕ_{1} and ϕ_{2} are best measured near the merger of the two black holes. …”
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    Census of transient orbital resonances encountered during binary inspiral by Ruangsri, Uchupol, Hughes, Scott A

    Published 2014
    “…Transient orbital resonances have recently been identified as potentially important to the inspiral of small bodies into large black holes. …”
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    Secular Spin–Orbit Resonances of Black Hole Binaries in AGN Disks by Gongjie Li, Hareesh Gautham Bhaskar, Bence Kocsis, Douglas N. C. Lin

    Published 2023-01-01
    “…Here, we study the role of secular spin–orbit resonance in the evolution of an sBH binary component around a supermassive BH (SMBH) in an AGN disk. …”
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    TOI-216b and TOI-216 c: two warm, large exoplanets in or slightly wide of the 2:1 orbital resonance by Huang, Chelsea, Sha, Lizhou, Ricker, George R., Vanderspek, Roland K., Seager, Sara, Daylan, Tansu, Dynes, Scott, Yu, Liang

    Published 2020
    “…Although high eccentricity tidal migration has been invoked to explain their proximity to their host stars, a handful reside in or near orbital resonance with nearby planets, suggesting a gentler history of in situ formation or disk migration. …”
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