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AGB Stars New Models:Lithium Production in the Galaxy and Magellanic Clouds

  • P. Ventura
Part of the Astrophysics and Space Science Library book series (ASSL, volume 255)

Abstract

The discovery in the Galaxy and in the Magellanic Clouds of several Asymptotic Giant Branch (AGB) sources which display a surface lithium abundance (log(ε(7 Li)) up to 4, where log(ε(7 Li)) = log(7 Li/H) + 12) which is much larger than those commonly observed in galactic giants (log(ε(7 Li)) < 0.5) (Abia et al. 1993; Smith & Lambert 1989, 1990; Smith et al. 1995) is a clear hint on the fact that AGB stars manufacture lithium, despite the fact that this latter is heavily destroyed within the interiors of stars via the reaction 7 Li + p

Keywords

Mass Loss Rate Core Mass Convective Model Large Magellanic Cloud Thermal Pulse 
These keywords were added by machine and not by the authors. This process is experimental and the keywords may be updated as the learning algorithm improves.

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Copyright information

© Springer Science+Business Media Dordrecht 2000

Authors and Affiliations

  • P. Ventura
    • 1
  1. 1.Osservatorio Astronomico di RomaMontePorzio Catone (RM)Roma

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