Program
February 16, 2016
9:40 | Welcome Address |
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9:45 – 10:15 | Bertrand Lefloch (IPAG) The ASAI view on the evolution of molecular complexity along the formation of sun-like stars |
10:15 – 10:45 | Tomoya Hirota (NAOJ) Hot water disk around Orion Source I |
10:45 – 11:15 | Izaskun Jimenez-Serra (UCL) The physical and chemical structure of low-velocity MHD shocks |
11:15 – 11:45 | Jose Cernicharo (ICMM) Carbon chemistry in evolved stars: The Nanocosmos project |
11:45 – 13:00 | Lunch |
13:00 – 13:30 | Evelyne Roueff (Paris) Isotopic fractionation of carbon, deuterium and nitrogen: a full chemical approach |
13:30 – 14:00 | Naoki Watanabe (Hokkaido U.) Experimental approach to ortho-to-para ratio of hydrogen and water molecules desorbed from ice at around 10 K |
14:00 – 14:30 | Toshiyuki Azuma (RIKEN) Cooling dynamics of negative carbon cluster ions studied by an ion storage ring |
14:30 – 15:00 | Charlotte Vastel (IRAP) New insights on the earliest phase of low-mass star forming regions |
15:00 – 15:30 | Coffee break |
15:30 – 16:00 | Yuri Aikawa (Tsukuba U.) Chemistry in the disk formation |
16:00 – 16:30 | Yoko Oya (U. Tokyo) A drastic change in the disk forming regions |
16:30 – 17:00 | Linda Podio (Arcetri) Sulfur chemistry in Class 0 disks and jets with ALMA |
17:00 – 17:30 | Jaime Pineda (MPI) From cores to disk: Just follow the gas |
17:30 – 18:00 | Hideko Nomura (TITEC) ALMA observations of CO gas depletion in the protoplanetary disk around TW Hya |
18:15 – 20:00 | Dinner |