Physics
Scientific paper
Nov 2000
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2000ign..confe..13c&link_type=abstract
Ionized Gaseous Nebulae. Mexico City November 21- 24, 2000, meeting abstract
Physics
Scientific paper
How the Galactic Bulge formed, what was the duration of this episode, are qu ite controversary subjects. It is even unclear wether stars are still forming there. These questions are generaly adressed with stars, but planetary nebulae are very apropriate tools to trace the Bulge history as well, due to the great variety of their progenitor lifetimes. In particular, because diferent elements are detectable in planetary nebulae and in stars, a combined analysis of the abundances patterns detected in stars and in planetary nebulae offers new insight in this problem. In long lived stars, most elements have their abundances unmodified and keep the fingerprints of the ISM when it was born. Analysing element abundances both in planetary nebulae and in stars allow thus to have a very good idea of the chemical enrichment of the ISM. We will see how we can understand these patterns in terms of supernovae of type II and type Ia explosions. Because the lifetimes of the progenitors of type II and type Ia supernovae are quite different, they offer very good chronometers for the Bulge evolution. As well, we will see how the abundances of elements synthetised in planetary nebulae progenitors can be unterstood in terms of recent star formation.
Acker Agnés
Cuisinier Francois
Köppen Joachim
Maciel Walter J.
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