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-====== The MaTYSSE team ====== 
  
-Gathering observers & theorists from the whole community, the MaTYSSE team is well set to efficiently tackle all issues addressed by this program. More specifically,​ our team include specialists of all domains involved in this program, ie stellar magnetic imaging & activity, magnetospheric accretion processes, formation & evolution of low-mass stars, exoplanets & planet migration, dynamos & stellar winds. ​ The full team is listed in the Table below.  ​ 
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-^ Partner ^ Team members ^ 
-| France | J-F Donati, E Hébrard,​ L Jouve, C Baruteau (IRAP, Toulouse), J Morin (LUPM, Montepellier),​ F Ménard, C Dougados, J Bouvier, J Ferreira, X Delfosse,​ X Bonfils, T Forveille (IPAG, Grenoble), I Boisse (LAM, Marseille), G Hébrard (IAP, Paris), G Chabrier (ENS, Lyon), S Brun (CEA, Saclay), A Morbidelli, A Crida (OCA, Nice) |  
-| Canada | R Doyon, E Artigau, D Lafreniere (UdM, Montreal), D Bohlender, C Marois (HIA, Victoria) |  
-| Brazil | SHP Alencar, G Franco (UFMG, Belo Horizonte), J Gregorio-Hetem (Sao Paulo) |  
-| CFHT | C Moutou | 
-| Taiwan | H Takami, SY Wang, H Shang (ASIAA, Taipei), SP Lai (NTHU, Hsinchu) |  
-| ESO | G Hussain |  
-| Ukraine | K Grankin, S Artemenko (CAO) |  
-| China | G Herczeg (NAO, Beijing), SH Gu (NAO, Kunming) |  
-| UK | I Baraffe, M Browning, S Matt (Exeter), S Mohanty, Y Unruh (Imperial), M Jardine, A Vidotto, R Fares, A Cameron, SG Gregory (StAndrews),​ K Rice (Edinburgh) |  
-| USA | A Dupree, N Brickhouse (CfA), M Romanova (Cornell), L Rebull, L Hillenbrand (Caltech)| ​ 
-| Italy | C Argiroffi, E Flaccomio (Palermo) |  
-| Switzerland | A Vidotto, F Pepe, F Bouchy, C Lovis (Geneve) |  
-| Portugal | P Figueira (CAUP, Porto) |  
project.1397825418.txt.gz · Last modified: 2014/04/18 14:50 by jdonati