activity
19992026
most citedMeasurement of stellar age from uranium decay

381 citations · 1.7k across the 22 of their papers we have counts for

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astro-ph2007★ 339 cited

First Stars VIII -- Enrichment of the neutron-capture elements in the early Galaxy

P. Francois, E. Depagne, V. Hill +12

Our aim is to measure accurate, homogeneous neutron-capture element abundances for the sample of 32 EMP giant stars studied earlier in this series, including 22 stars with [Fe/H] $…

astro-ph2006★ 115 cited

First stars X. The nature of three unevolved Carbon-Enhanced Metal-Poor stars

T. Sivarani, T. C. Beers, P. Bonifacio +13

From high-resolution VLT/UVES spectra (R~43,000), we determine abundances or upper limits for Li, C, N, O, and other important elements, as well as 12C/13C isotopic ratio for three…

astro-ph2004★ 69 cited

Cu and Zn in the early Galaxy

G. Bihain, G. Israelian, R. Rebolo +2

We present Cu and Zn abundances for 38 FGK stars, mostly dwarfs, spanning a metallicity range between solar and [Fe/H] =-3. The abundances were obtained using Kurucz's local therma…

astro-ph2001★ 381 cited

Measurement of stellar age from uranium decay

R. Cayrel, V. Hill, T. Beers +10

The ages of the oldest stars in the Galaxy indicate when star formation began, and provide a minimum age for the Universe. Radioactive dating of meteoritic material and stars relie…

astro-ph2000★ 11 cited

Intrinsic colour calibration for F, G, K stars

Piercarlo Bonifacio, Elisabetta Caffau, Paolo Molaro

We derive an intrinsic colour calibration for F--K stars using broad band Johnson colours and line indices KP and HP2. Through this calibration we can determine E(B-V) of an indivi…

astro-ph1999★ 1 cited

The Galactic Lithium Evolution Revisited

D. Romano, F. Matteucci, P. Molaro +1

The evolution of the 7Li abundance in the Galaxy has been computed by taking into account several 7Li sources: novae, massive AGB stars, C-stars, Type II SNe and GCRs. The theoreti…