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DH Tau is a young (sim;1 Myr) classical T Tauri star. It is one of the few young PMS stars known to be associated with a planetary mass companion, DH Tau b, orbiting at large separation and detected by direct imaging. DH Tau b is thought to be accreting based on copious Ha emission and exhibits v...


Wolff, S.G.Ménard, F.Caceres, C.Lefèvre, C.Bonnefoy, M.Cánovas, H.Maret, S.Pinte, C.Schreiber, M.R.Plas, G.V.D.[An Upper Limit on the Mass of the Circumplanetary Disk for DH Tau b]An Upper Limit on the Mass of the Circumplanetary Disk for DH Tau b

Lazareff, B.Lachaume, Regis.Berger, Jean-Philippe.Kluska, J.Le Bouquin, J.-B.Benisty, M.Malbet, Fabien.Koen, C.Pinte, C.Thi, W.-F.Absil, O.[Structure of Herbig AeBe disks at the milliarcsecond scale : a statistical survey in the H band using PIONIER VLTI.]Structure of Herbig AeBe disks at the milliarcsecond scale : a statistical survey in the H band using PIONIER VLTI.

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