|
(Image copyright: Bernd Müller, Augsburg) |
Welcome to the homepage ofAchim Weiss |
Stellar evolution of low- and intermediate-mass stars:
Low-mass stars: evolution, physics (mixing processes, nucleosynthesis)
intermediate-mass stars: Asymptotic Giant Branch (evolution, mixing, nucleosynthesis), Cepheids (convection, mass)
The Sun (interior structure, seismology, solar abundance problem)
The Sun (interior structure, seismology, solar abundance problem)
The Sun (interior structure, seismology, solar abundance problem)
Asteroseismology (giants, clusters, massive stars: models for seismic analysis; CoRoT, KEPLER, PLATO)
Clusters, globular and open (age, composition, sub-populations, laboratories for stellar structure theory)
Stellar ages (clusters, field stars, individual stars)
Dynamical and energetic events in stars (core helium flash, thermal pulses, convection, semiconvection, hydrostatic and -dynamic approach)
Evolution of Pop III stars (low-mass, composition, extremely metal-poor stars in the galactic halo)
Population synthesis: stellar models as input, AGB stars: evolutionary state and colours
AGB- and post-AGB-evolution (see above; and - how to produce good models for AGB-stars?)
Fingerprint: 52E4 B09F 341F 0BB1 2532 82C4 E5C5 EE81 A2E2 3BD0