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

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dc.contributor.authorFaramaz, V.
dc.contributor.authorErtel, S.
dc.contributor.authorHaworth-Booth, Mark
dc.contributor.authorCuadra Stipetich, Jorge Rodrigo
dc.contributor.authorSimmonds, C.
dc.date.accessioned2021-05-22T01:10:23Z
dc.date.available2021-05-22T01:10:23Z
dc.date.issued2017
dc.format.extent14 páginas
dc.fuente.origenConveris
dc.identifier.doi10.1093/mnras/stw2846
dc.identifier.eissn1365-2966
dc.identifier.issn0035-8711
dc.identifier.urihttps://doi.org/10.1093/mnras/stw2846
dc.identifier.urihttps://repositorio.uc.cl/handle/11534/58895
dc.issue.numeroNo. 2
dc.language.isoen
dc.nota.accesoContenido completo
dc.pagina.final2365
dc.pagina.inicio2352
dc.revistaMonthly Notices of the Royal Astronomical Societyes_ES
dc.rightsacceso abierto
dc.titleInner mean-motion resonances with eccentric planets: a possible origin for exozodiacal dust cloudses_ES
dc.typeartículo
dc.volumenVol. 465
sipa.codpersvinculados1012996
sipa.codpersvinculados3855
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