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Melendez, J. Ramos, M. Bonavita, M. Bonnefoy, M. Cudel, M. Feldt, M. Janson, M. Kasper, M. Keppler, M. Langlois, M. Lombart, M.R. Mayer, M. Samland, N. Engler, P. Delorme, R. Claudi, R. Galicher, R. Gratton, R. Ligi, S. Daemgen, S. Desidera, S. Hunziker, S. Mazevet, S. Peretti, S. Petrus, T. A. Pacheco, T. Moulin, T.O.B. Schmidt, T. Stolker, V. D'Orazi, W. Brandner","submitted_at":"2020-12-10T10:45:34Z","abstract_excerpt":"Sirius-like systems are wide binaries composed of a white dwarf (WD) and a companion of a spectral type earlier than M0. The WD progenitor evolves in isolation, but its wind during the AGB phase pollutes the companion surface and transfers some angular momentum. Within SHINE survey that uses SPHERE at the VLT, we acquired images of HD2133, HD114174, and CD-567708 and combined this data with high resolution spectra of the primaries, TESS, and literature data. We performed accurate abundance analyses for the MS. 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