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Browsing by Author "Decressin, T."
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The chemical composition of TS 01, the most oxygen-deficient planetary nebula AGB nucleosynthesis in a metal-poor binary star
Stasinska, G.; Morisset, C.; Tovmassian, G.; Rauch, T.; Richer, M.G.; Pena, M.; Szczerba, R.; Decressin, T.; Charbonnel, C.; Yungelson, L.; Napiwotzki, R.; Simon-Diaz, S.; Jamet, L. (2010)The planetary nebula TS 01 (also called PN G 135.9+55.9 or SBS 1150+599A) with its record-holding low oxygen abundance and its double degenerate close binary core (period 3.9 h) is an exceptional object located in the ... -
Superbubble dynamics in globular cluster infancy. I. How do globular clusters first lose their cold gas?
Krause, M.; Charbonnel, C.; Decressin, T.; Meynet, G.; Prantzos, N.; Diehl, R. (2012-10-05)The picture of the early evolution of globular clusters has been significantly revised in recent years. Current scenarios require at least two generations of stars of which the first generation (1G), and therefore also the ... -
Superbubble dynamics in globular cluster infancy. II. Consequences for secondary star formation in the context of self-enrichment via fast-rotating massive stars
Krause, M.; Charbonnel, C.; Decressin, T.; Meynet, G.; Prantzos, N. (2013-04-12)Context. The self-enrichment scenario for globular clusters (GC) requires large amounts of residual gas after the initial formation of the first stellar generation. Recently, we found that supernovae may not be able to ...