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Article 2017-06

An Upper Limit on the Mass of the Circumplanetary Disk for DH Tau b

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

Repositorio Universidad Andrés Bello

Circumstellar matter

Planetary systems

Stars: individual (DH Tau)

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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

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Probing the final stages of protoplanetary disk evolution with ALMA

An Upper Limit on the Mass of the Circumplanetary Disk for DH Tau b

Descubre y comparte nuestro conocimiento público

Resultados de búsqueda

Probing the final stages of protoplanetary disk evolution with ALMA

[Probing-the-final-stages-of-protoplanetary-disk-evolution-with-ALMA.pdf]

An Upper Limit on the Mass of the Circumplanetary Disk for DH Tau b

[Wolff_S_An_Upper_Limit.pdf]