Summary
-
extension of studies linked to newly developed scenario of the origin of field
halo stars and of globular clusters;
-
acquisition of high resolution spectroscopic data with UVES on ESO's VLT
in order to construct models of the chemical evolution of e.g. AGB stars;
-
study of the formation of planetary nebulae;
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eduction of space data (e.g. ISO) and preparation in the contact of future
missions (e.g. Herschel).
Partners involved:
Université
de Liège
Katholieke Universiteit Leuven
Royal Observatory of Belgium
Links
Web pages:Sandrine Sohy
Last modification: June 7, 2004
