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Modelling of AGB stars in the LMC
Asymptotic giant branch (AGB) stars are major contributors to both the chemical enrichment of the interstellar medium and the integrated light of galaxies. Despite its... -
Modelling of Magellanic Cloud C/O stars
Mass loss is one of the fundamental properties of Asymptotic Giant Branch (AGB) stars, and through the enrichment of the interstellar medium, AGB stars are key players in the... -
Stellar evolution. II. Post-AGB
We present a set of evolutionary tracks for central stars of planetary nebulae in the range from 0.53 to 0.94M_{sun}. These models are based on extensive stellar evolution... -
Low-mass stars
(no description available)
