activity
20032008
most citedA probable stellar solution to the cosmological lithium discrepancy

322 citations · 546 across the 4 of their papers we have counts for

collaborators
Showing astro-phShow all

6 papers · 1 filter

astro-ph2008

New high resolution synthetic stellar libraries for the Gaia Mission

R. Sordo, A. Vallenari, J. C. Bouret +12

High resolution synthetic stellar libraries are of fundamental importance for the preparation of the Gaia Mission. We present new sets of spectral stellar libraries covering two sp…

astro-ph2007224 cited

Atomic Diffusion and Mixing in Old Stars I. VLT/FLAMES-UVES Observations of Stars in NGC 6397

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

We present a homogeneous photometric and spectroscopic analysis of 18 stars along the evolutionary sequence of the metal-poor globular cluster NGC 6397 ([Fe/H] = -2), from the main…

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-ph2005

Pristine CNO abundances from Magellanic Cloud B stars II. Fast rotators in the LMC cluster NGC 2004

A. J. Korn, M. F. Nieva, S. Daflon +1

We present spectroscopic abundance analyses of three main-sequence B stars in the young Large Magellanic Cloud cluster NGC 2004. All three targets have projected rotational velocit…

astro-ph2004

Higher-order Balmer line indices in alpha/Fe-enhanced stellar population models

Daniel Thomas, Claudia Maraston, Andreas Korn

We have computed the higher-order Balmer absorption line indices Hgamma and Hdelta (Worthey & Ottaviani 1997) for stellar population models with variable element ratios. The respon…