Molecular Line Observations of Protoplanetary Disks

E. Chapillon (1, 2) , Anne Dutrey (1) , Thomas Henning (3) , S. Guilloteau (1) , Valentine Wakelam (1) , F. Hersant (4) , Frédéric Gueth (2) , Vincent Piétu (2, 5) , Nagayoshi Ohashi , Y. Boehler (1) , Ralf Launhardt (3) , Dimitry Semenov , Katharina Schreyer , Michel Guélin (2) , Bérengère Parise (6)

1 AMOR 2013
2 IRAM - Institut de RadioAstronomie Millimétrique
3 MPIA - Max-Planck-Institut für Astronomie
4 FORMATION STELLAIRE 2013
5 IPAG - Institut de Planétologie et d'Astrophysique de Grenoble
6 MPIFR - Max-Planck-Institut für Radioastronomie

We summarize in this poster a long-term study of the chemistry as a powerful tool to constrain the protoplanetary disk physics. Most of the above results were obtained in the frame of the CID (Chemistry In Disks) consortium.

Domaines: Astrophysique stellaire et solaire [astro-ph.SR]; Astrophysique stellaire et solaire [astro-ph.SR]; Cosmologie et astrophysique extra-galactique [astro-ph.CO]; Cosmologie et astrophysique extra-galactique [astro-ph.CO]

E. Chapillon, Anne Dutrey, Thomas Henning, S. Guilloteau, Valentine Wakelam, et al.. Molecular Line Observations of Protoplanetary Disks. Protostars and Planets VI, Heidelberg, July 15-20, 2013. Poster #2S023, 2013, Heidelberg, Germany. ⟨hal-00880565⟩