activity
20052007
most citedA probable stellar solution to the cosmological lithium discrepancy

322 citations · 680 across the 7 of their papers we have counts for

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Showing 2006 · astro-phShow all

6 papers · 2 filters

astro-ph2006134 cited

Disentangling the Hercules stream

T. Bensby, M. S. Oey, S. Feltzing +1

Using high-resolution spectra of nearby F and G dwarf stars, we have investigated the detailed abundance and age structure of the Hercules stream. We find that the stars in the str…

astro-ph2006

Hercules stream stars and the metal-rich thick disk

T. Bensby, M. S. Oey, S. Feltzing +1

Using the MIKE spectrograph, mounted on the 6.5 m Magellan/Clay telescope at the Las Campanas observatory in Chile, we have obtained high-resolution spectra for 60 F and G dwarf st…

astro-ph2006

New Abundances for Old Stars - Atomic Diffusion at Work in NGC 6397

A. J. Korn, F. Grundahl, O. Richard +5

A homogeneous spectroscopic analysis of unevolved and evolved stars in the metal-poor globular cluster NGC 6397 with FLAMES-UVES reveals systematic trends of stellar surface abunda…

astro-ph2006322 cited

A probable stellar solution to the cosmological lithium discrepancy

A. J. Korn, F. Grundahl, O. Richard +5

The measurement of the cosmic microwave background has strongly constrained the cosmological parameters of the Universe. When the measured density of baryons (ordinary matter) is c…

astro-ph2006

Analysis of the Luminosity-Stellar Mass-Metallicity Relation in cosmological simulations

Maria Emilia De Rossi, Patricia Beatriz Tissera, Cecilia Scannapieco

We study the Luminosity-Metallicity Relation and the Stellar Mass-Metallicity Relation by performing chemo-dynamical simulations in a cosmological scenario. Our results predict a t…

astro-ph2006

Evolution of the Luminosity-Metallicity-Stellar Mass correlation in a hierarchical scenario

Maria Emilia De Rossi, Patricia Beatriz Tissera, Cecilia Scannapieco

We study the evolution of the Stellar Mass-Metallicity Relation and the Luminosity-Metallicity Relation by performing numerical simulations in a cosmological framework. We find tha…