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Program

February 16, 2016

9:40                

Welcome Address

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