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ProgramJanuary 12 – Morning
- 09:00 – 09:10 - Welcome : A.Dutrey - 09:10 – 09:35 – ALMA/C4 : L.Testi - 09:35 – 10 :00 – NOEMA : F.Gueth
- Chair : Some Fundamental Questions – 10 min – C.Ceccarelli - Which Chemical Models for What ? - 25 min – A.Vasyunin - Strengths and Limitations of Models – 25 min – R. Ruaud
- Pre-stellar Cores – 20 min - C.Vastel - Class 0/I - 20min – S.Maret - Class II /transition disks - 20 min – C.Walsh
January 12 – Afternoon
- Chair : Some Fundamental Questions – 10 min – P.Caselli - What Chemical Model Predicts - 25 min – D.Semenov - Pre-stellar cores – 20 min – S.Kong - Class 0/I - 20 min – K.Furuya - Class II/disks – 20 min – R.Teague - ALMA recent results - 20 min - K.Oberg, tentative
- Low-Mass Stars – 20 min – A. Coutens - High- Mass Stars – 20 min - F .Fontani - Round Table 1 – « Chemistry » - 20min - TBD
January 13 – Morning
- Chair : Some Fundamental Questions – 10 min – C.Codella - Review of Disk Formation - 20 min – B.Commerçon - Chemistry during disk formation – 20 min ; Y.Aikawa, tentative
- Class 0/I - 20 min – N.Ohashi, tentative - Sulfur chemistry in class 0 disks and jets - 20 min – L.Podio - High-Mass Stars - 20 min - M.Beltran
- Chair : « Pro & Con » – 10 min – E.Van Dishoeck, tentative - Retrieving data from the ALMA archive : a user point of view – 25 min - S. Guilloteau - General Discussion I
January 13 – Afternoon
- Chair : Some Fundamental Questions - 10min – TBD - Stars & Disks : general scheme – 25 min - M. Kama - Class I – 20min - J.Joergensen, - Class II – 20 min - I.Cleeves - Multiple stellar systems – 20min – Y.W.Tang - Gas in Evolved Disks – 20 min – A. Kospal
- Measuring the temperature – 20 min - U.Gorti - Measuring the gas mass – E.Chapillon - Round Table 2 – « Disks » - 20min - TBD
Presentations and discussions : + Short Introduction by the chair (10 min) : - Present 3-5 transparencies with a list of important issues and pending problems - These transparencies can be also used during the round table + Some points to address during the Round Tables : - What do we need ? - Sensitivity ? - Angular Resolution ? - Detailed studies versus suveys ?
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