activity
19972008
most citedNucleosynthetic signatures of the first stars

566 citations · 570 across the 8 of their papers we have counts for

collaborators
Showing astro-phShow all

14 papers · 1 filter

astro-ph20082 cited

Reality of Moving Groups in the Galaxy

G. M. De Silva, K. C. Freeman, J. Bland-Hawthorn +1

The existence of old dispersed stellar groups within the Milky Way disk is still controversial. Are they the debris of ancient star-forming aggregates, or short-lived artifacts of…

astro-ph2005566 cited

Nucleosynthetic signatures of the first stars

Anna Frebel, Wako Aoki, Norbert Christlieb +16

The chemically most primitive stars provide constraints on the nature of the first stellar objects that formed in the Universe; elements other than hydrogen, helium and traces of l…

astro-ph2003

Uncertainties in stellar abundance analyses

Martin Asplund

Over the last half-century quantitative stellar spectroscopy has made great progress. However, most stellar abundance analyses today still employ rather simplified models, which ca…

astro-ph20031 cited

Globular cluster abundances in the light of 3D hydrodynamical model atmospheres

Martin Asplund

The new generation of 3D hydrodynamical model atmospheres have been employed to study the impact of a realistic treatment of stellar convection on element abundance determinations…

astro-ph2003

New generations of stellar model atmospheres

Martin Asplund

Stellar model atmospheres form the basis for any element abundance determination and hence are crucial ingredients for studies of stellar, galactic and cosmic evolution. With recen…

astro-ph20031 cited

Radiative transfer in 3D model stellar atmospheres

Martin Asplund, Remo Collet

Recently 3D hydrodynamical simulations of stellar surface convection have become feasible thanks to advances in computer technology and efficient numerical algorithms. Available ob…