Abstract
Les observations polarimetriques de la nova recurrente RS Oph, realisees durant son eruption de 1985, sont presentees. Une polarisation lineaire variable est observee, indiquant la presence d'une polarisation intrinseque. Une separation des polarisations interstellaire et intrinseque montre que l'angle de position de la polarisation lineaire est aligne avec la structure de jet radio observee en VLBI
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