Inner mean-motion resonances with eccentric planets: a possible origin for exozodiacal dust clouds

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Inner mean-motion resonances with eccentric planets- a possible origin for exozodiacal dust clouds .pdf(4.57 MB)
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2017
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https://doi.org/10.1093/mnras/stw2846
 https://repositorio.uc.cl/handle/11534/58895
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