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Treating dynamical stability as an observable: a 5:2 mean motion resonance configuration for the extrasolar system HD 181433
Giammarco CampanellaVolume:
418
Year:
2011
Language:
english
Pages:
11
DOI:
10.1111/j.1365-2966.2011.19553.x
File:
PDF, 6.32 MB
english, 2011