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Population III and metal-free star formation -
- Primordial building blocks: from dark matter halos to the first stars
- Population III stars: formation and evolution
- Population III to Pop. II transition: chemical vs. radiative feedback
- Searches for Pop. III and very metal-poor populations in the distant universe
Metal-poor IMFs, stellar evolution, and star-formation histories -
- Local relics of primordial star formation: the Milky Way halo and
local dwarfs
- Star-formation histories at low metallicity in dwarf galaxies
- Stellar evolution at low metallicity
- Low-metallicity star clusters and the IMF in metal-poor environments
Low-metallicity star formation in local dwarf galaxies -
Dust and gas as seeds for metal-poor star formation -
- Dust in low-metallicity ISMs
- The gas phase in a low-metallicity ISM
- Molecule formation in primordial conditions
Explosive events in low-metallicity environments: SNe and GRBs -
- SNe and their evolution in a metal-poor ISM
- Low-mass and metal-poor GRB host galaxies
Metal enrichment, chemical evolution, and feedback -
- Chemical evolution and feedback constraints
on galaxy formation and IGM enrichment
- Feedback and mechanical energy input in chemical and stellar evolution
- Damped Lyman-alpha systems as probes of chemical evolution over
cosmological timescales
Dwarf galaxies in a cosmological context:
proxies for primordial star formation?
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