Autor:
Wolff, S.G.
Ménard, F.
Caceres, C.
Lefèvre, C.
Bonnefoy, M.
Cánovas, H.
Maret, S.
Pinte, C.
Schreiber, M.R.
Plas, G.V.D.
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...
Enlace original:
http://repositorio.unab.cl/xmlui/handle/ria/5026
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
